The galaxy presents an elliptical morphology, appearing somewhat elongated along its major axis. Its core is highly luminous and concentrated, suggesting a significant population of older stars or possibly an active galactic nucleus, though this is difficult to ascertain from a single image. The light distribution appears relatively smooth, with little evidence of spiral arms or distinct substructures. Some faint, diffuse extensions are present in the outer regions, hinting at a possible interaction or tidal disturbance, though the contrast is low. The overall color is indicative of a galaxy dominated by older stellar populations.
