  We study the quantum gravity modification of the Kuroda-Papapetrou model
induced by the running of the Newton's constant at high energy in Quantum
Einstein Gravity. We argue that although the antiscreening character of the
gravitational interaction favours the formation of a naked singularity, quantum
gravity effects turn the classical singularity into a "whimper" singularity
which remains naked for a finite amount of advanced time.
