Welcome scains25, your question presumes that somehow we have precise measurements of dark matter, and we don't. You will often see cutting-edge research in Astronomy say that there is an indication of something, and that implies that further study will be needed to get details. So the answer, rather vaguely expressed is that the dark matter that is dense enough to support the roughly constant rotation velocity doesn't extend much beyond the dense stars in M31. It's shape may be distorted by recent mergers and a pass-through of another galaxy or two (M32 & NGC205), but we don't have enough precision to say for sure. The dark matter halo around M31 DOES extend perhaps a third of the way to the Milky Way, but it gets thinner as it extends out, and again the specifics are only loosely known.
Forming opinions as we speak