  A regular rotating MOG (modified gravity) compact object is derived that
reduces to the Kerr black hole when the parameter $\alpha=0$. Physical
consequences of the dark compact object, which is regular everywhere in
spacetime for $\alpha > \alpha_{\rm crit}=0.674$ and is a rotating Kerr-MOG
black hole for $\alpha < \alpha_{\rm crit}$ are investigated.
