  We study shadow aspects of superentropic black holes in four dimensions.
Using Hamilton-Jacobi formalism, we first get the null geodesic equations. In
the celestial coordinate framework relying on fixed positions of observers, we
investigate the shadow behaviors in terms of the mass and the cosmological
scale variation parameters. Among others, we obtain ellipse shaped geometries
contrary to usual black hole solutions. Modifying the ordinary relations
describing geometrical observables, we discuss the size and the shape
deformation parameters of these non-trivial geometric forms. Due to horizonless
limits associated with certain mass values, we explore the shadow of the naked
singularity of such black holes.
