  In this paper, we study the dynamics of a test particle around a regular
black hole (BH) in a non-minimal Einstein Yang Mills (EYM) theory and examine
the BH shadow. The EYM theory is a non-minimally coupled theory in which
curvature couples to non-Abelian gauge fields. We investigate particle motion
with parameters in EYM BH for massless and massive particles. This work
provides the horizon structure, photon radius and inner stable circular orbit
(ISCO) of a mass particle with EYM BH parameters. An analysis is provided of
the effective potential as well as the possible orbits for test particles under
various EYM BH parameters values. In timelike radial geodesics, we find that
for smaller values of magnetic charge, particles following a timelike radial
geodesic are hastier in EYM BH, and hence arrive at the center faster than
those traveling a Schwarzschild BH geodesic. However, at larger values of the
magnetic charge, the inverse effect is observed. The effect of model parameters
is investigated in order to study the ISCO, photon radius, orbit stability
(Lyapunov exponent), and effective force on particles for the BH in the EYM
theory. Finally, we investigate the BH shadow. We find that higher magnetic
charge values and non-minimal coupling parameters result in smaller shadow
radius values.
