The placement of the center of the map is messed up, but it's nobody's mistake. From chapter 4 of The Surface of Mars:
The elevation difference between the two hemispheres
offsets the planet’s center of figure from its center of
mass by 2.986 km as measured along the polar axis
Regarding the question that is in the title ("Why are the hemispheres so different?"), this sharp contrast between the Northern and Southern hemispheres is known as the Martian dichotomy.
The elevation on Mars follows a bimodal distribution. That is most of the land is either 4 km under the mean altitude or 1.5 km above the mean altitude.
But not only is the altitude different between the two hemispheres, but the crustal thickness and the number of impact craters are also very different.
There are several competing hypotheses to explain the dichotomy. Here are a few.
Part of the crust was overturned
Very early in the history of Mars, there was a magma ocean that crystallized. Solomon et al. (2005) suggest that the top the mantle ended up denser than what was underneath, and it flipped.
There used to be active margins
By analogy with the dichotomy seen on Earth between oceans and continents, Sleep (1994) suggests that the northern hemisphere may be the result of new crust being generated and spreading from the center. The limit between the two areas would have been an active margin, similar to the Andes where the oceanic crust drops under the continental crust.
However, this would result in the formation of magnetic stripes that are observed in the southern rather than in the northern hemisphere.
Thermal convection in the mantle
As suggested by Zhong and Zuber (2001), there might have been strong convection in the mantle with a single convection cell.
These models succeed in reproducing some differences between the two hemispheres.
A giant impact in the northern hemisphere
Wilhelms and Squyres (1984) suggest that a giant impact very early in the history of Mars might have caused the northern depression. They also indicate the location of the impact.
However, no thinning of the crust has been found there, like what is observed for younger and smaller craters. The ring deposits that such an impact would have created are missing. The edge of the northern plains are very irregular, when impact craters tend to be somewhat circular.
A giant impact in the southern hemisphere
Leone et al. (2016) propose that the dichotomy is the result of an impact in the southern hemisphere and that the result of the impact in more crust, rather than missing crust.
A few not quite as giant impacts
Explaining the irregular boundary between the two areas is rather difficult with a single impact, so Frey and Schultz (1988) suggest that a few big impacts might have caused the peculiar geography of Mars.
However, this hypothesis doesn't completely explain why the impact basin isn't circular.
So the question of the martian dichotomy is still open and doesn't have a definitive answer yet.