  In this work we have obtained a charged black hole solution in the presence
of perfect fluid dark matter (PFDM) and discuss its energy conditions. The
metric corresponding to the rotating avatar of this black hole solution is
obtained by incorporating the Newman-Janis algorithm. We then compute two types
of circular geodesics, namely, the null geodesics and time-like geodesics for
this rotating spacetime geometry. For the case of time-like geodesics, we
consider both neutral as well as charged massive particles. The effective
potentials of the corresponding circular geodesics has also been studied. We
then present our results by graphically representing the collective effects of
the black hole parameters, namely, the charge of the black hole ($Q$), spin
parameter ($a$) and the PFDM parameter ($\alpha$) on the energy ($E$), angular
momentum ($L$) and effective potential ($V_{eff}$) of the concerned particle.
Finally, we discuss the Penrose process in order to study the negative energy
particles having possible existence within the ergosphere, and which in turn
leads to the energy gain of the emitted particle.
