  We find a rotating Kaluza-Klein black hole solution with a squashed $S^3$
horizon in five dimensions. This is a Kerr counterpart of the charged one found
by Ishihara and Matsuno (hep-th/0510094) recently. The space-time is geodesic
complete and free of naked singularity. Its asymptotic structure is a twisted
$S^1$ fiber bundle over a four dimensional Minkowski space-time. We also study
the mass and thermodynamics of this black hole.
