The galaxy presents as a centrally concentrated system with a generally smooth appearance. The light is dominated by an elliptical morphology, with isophotes that are generally round, showing only slight deviations from perfect circularity. Its color index suggests a composition of older stellar populations and a low rate of current star formation. There is no strong evidence for spiral arm structure or a prominent disk. Faint tidal features or interactions may be present, warranting further investigation to ascertain if the galaxy has undergone recent or ongoing mergers or disturbances. The angular size of the galaxy is relatively small, corresponding to a physical radius of approximately 5 kpc.
