  We investigate the spin dynamics of a millisecond pulsar (MSP) in compact
orbit around a Kerr-like massive black hole with an general mass quadrupole. We
use the Mathisson-Papetrou-Dixon formulation to compute the orbital and spin
evolution of the MSP, accounting for the non-linear interaction of the pulsar's
energy-momentum tensor on the background spacetime metric. We investigate how
the MSP spin and BH quadrupole moment manifest in the pulsar spin-orbital
dynamics. We discuss the astrophysical observational implications of these spin
and orbital dynamics on the timing of a radio pulsar in an Extreme Mass Ratio
Binary, e.g. a Galactic Centre pulsar. In particular, notable timing variations
in the Einstein delay and Roemer delay are observed, along with modifications
to the pulsar pulse profile.
