Neutron stars structure is highly composite, in fact for the core of pulsars like magnetars is yet more or less unknown.
Neutron stars have an atmosphere of almost electron and plasma gas (sometimes liquid), that even if few cm thick can generate great magnetic field, having plasmon resonances and so on and a rich spectrum... So here you have electrons and finite nuclei (with protons and neutrons)
Then the crust of the neutron star can be divided into outer and inner crust. The outer crust is roughly half a km wide ad made mostly of a lattice of completely polarized finite nuclei. Usally (but not always) neutron rich. But you have again the same order of magnitude of protons and neutrons.
The inner crust runs deep for a couple of km and it is made mostly by a sea of neutrons but have a lot of proton "impurities" that condense to form bulges of protons. The ratio is about 50 condensed protons to 1000 of neutrons in most models.
Then you have the core, divided in
outer core, 4/5 km deep, made by neutrons, but again not so few protons created by the neutrino emission for cooling of the stars toghether with muons
and the misterious inner core, also approx 5 km deep, with a still unknown composition, but always with some charged material in the center: in most models toghether with p and n exotic baryons such as hyperions, but also condensed pions, kaons or even free quarks.
Above all, take into account that the neutron star is a very dynamic environment, like in a star there are a lot of nuclear reactions going on, mostly because it have to find ingenuous way to cool itself, but in such a system also weak force-based reactions are feasible and so the components, and even their charge (due to the weak-force driven reactions), change dynamically.