The galaxy presents as a centrally concentrated system with a smooth light distribution, suggesting a relatively high degree of symmetry. Its morphology is consistent with an elliptical or lenticular type galaxy, exhibiting a bulge-dominated structure. The core region displays a bright, concentrated luminosity, indicative of a high stellar density and potentially a supermassive black hole at the center. Moving outwards from the core, the galaxy exhibits a gradual decline in surface brightness. The outer regions appear more diffuse, with a somewhat amorphous halo. There is some evidence of a very subtle disc, however, the image is not high-resolution enough to definitively classify if it has features, or just a general flattening. The overall color of the galaxy is slightly yellow, which implies a population of older stars. There may be some indications of minor tidal disturbances, although the image quality limits conclusive identification of merging events.
