  We examine the shadow of a rotating Kaluza-Klein black hole in Einstein
gravity coupled to a Maxwell field and a dilaton. The size and the shape of the
shadow depend on the mass, the charge, and the angular momentum of the compact
object. For a given mass, the size increases with the rotation parameter and
decreases with the electric charge. The distortion with respect to the non
rotating case grows with the charge and the rotation parameter. For fixed
values of these parameters, the shadow is slightly larger and less deformed
than in the Kerr-Newman case.
