  We consider the geodesic motions in the Kerr-Sen-AdS$_4$ spacetime. We obtain
the equations of motion for light rays and test particles. Using the parametric
diagrams, we shown some regions where the radial and latitudinal geodesic
motions are allowed. We analyse the impact of parameter related to dilatonic
scalar on the orbit and find that it will result in more rich and complex
orbital types.
