  In this paper, we have investigated the dynamics of magnetized particles
around 4-D Einstein-Gauss-Bonnet black hole immersed in an external
asymptotically uniform magnetic field. We have shown that the magnetic
interaction parameter responsible for circular orbits decreases for negative
values of the Gauss-Bonnet parameter $\alpha$ and the range where magnetized
particle's stable circular orbits are allowed increases for the positive values
of the parameter $\alpha$. The study of the collisions of magnetized, charged
and neutral particles has shown that the center-of-mass energy of the particles
increases in the presence of positive Gauss-Bonnet parameter. Finally, we show
how the magnetic interaction and Gauss-Bonnet parameter may mimic the effect of
rotation of the Kerr black hole giving the same ISCO radius for magnetized
particles. Detailed analysis of the ISCO show that spin of Kerr black hole can
not be mimicked by the effects of magnetic interaction and the Gauss-Bonnet
parameters when $\alpha<-4.37$ and the spin parameter $a > 0.237$.
