  In this essay we examine the gravitational collapse of a nonrelativistic
charged perfect fluid interacting with a dark energy component. Given a simple
factor for the energy transfer, we obtain a nonsingular interior solution which
naturally matches the Reissner-Nordstr\"om-de Sitter exterior geometry. We also
show that the interacting parameter is proportional to the overall charge of
the final black hole thus formed. For the case of quasi-extremal
configurations, we propose a statistical model for the entropy of the collapsed
matter. This entropy extends Bekenstein's geometrical entropy by an additive
constant proportional to the area of the extremal black hole.
