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We examine the shadow of a rotating Kaluza-Klein black hole in Einsteingravity coupled to a Maxwell field and a dilaton. The size and the shape of theshadow depend on the mass, the charge, and the angular momentum of the compactobject. For a given mass, the size increases with the rotation parameter anddecreases with the electric charge. The distortion with respect to the nonrotating case grows with the charge and the rotation parameter. For fixedvalues of these parameters, the shadow is slightly larger and less deformedthan in the Kerr-Newman case.

Shadow cast by a Kaluza-Klein spinning dilaton black hole