The galaxy presents as a relatively compact object with a notable degree of rotational symmetry. Its morphology suggests a flattened disk structure viewed at a moderate inclination. The central region exhibits a bright, concentrated core, potentially indicative of a bulge component. Faint spiral arm structures are possibly present, but not sharply defined, appearing somewhat diffuse and tightly wound around the central bulge. There are hints of tidal disruption, specifically a light bridge across the galaxy's central core that presents at a sharp perpendicular to the plane of the disk. The galaxy displays a color gradient, appearing bluer in the outer disk regions and redder towards the core, which may imply younger stellar populations in the periphery and older populations in the center.
