  We present a spinning black hole solution in $d$ dimensions with a maximal
number of rotation parameters in the context of the Einstein-Maxwell-Dilaton
theory. An interesting feature of such a solution is that it accommodates
Lifshitz black holes when the rotation parameters are set to zero. We verify
the rotating nature of the black hole solution by performing the quasi-local
analysis of conserved charges and defining the corresponding angular momenta.
In addition, we perform the thermodynamical analysis of the black hole
configuration, show that the first law of thermodynamics is completely
consistent, and obtain a Smarr-like formula. We further study the thermodynamic
stability of the constructed solution from a local viewpoint, by computing the
associated specific heats, and from a global perspective, by using the
so-called new thermodynamic geometry. We finally make some comments related to
a pathology found in the causal structure of the obtained rotating black hole
spacetime and compute some of its curvature invariants.
