For something orbiting a nucleus, the only parameters that matter are electric charge and mass.
This stuff was figured out in the 1920s, and is taught in a year or two of undergraduate physics. The examples are usually an electron orbiting a proton (the hydrogen atom), but work just as well for muons, or anything else. It's only once you get inside the atom that you get into more advanced stuff.
Not a physicist. But if I understand correctly, it fits the same equations the electron would, except you have to use the proton mass instead of the electron mass, which means it's much closer in. The remaining electron (I think) doesn't have Pauli exclusion with the anti-proton, so it looks like the electron in a hydrogen atom. (Since it's much further out, it sees the effective charge of +1 for the "nucleus" of two protons and an anti-proton.)