The galaxy presents as a moderately bright object with a seemingly elliptical morphology. The central region exhibits a high surface brightness, suggesting a significant concentration of stars and potentially a supermassive black hole at its core. Fainter, diffuse extensions are visible emanating from the central region, indicating a disk-like structure viewed at a relatively high inclination. There is evidence of some irregular structure or tidal features, particularly on one side, hinting at possible past interactions or ongoing minor disturbances from smaller satellite galaxies. The overall color appears somewhat redder, suggesting an older stellar population and possibly a lower rate of ongoing star formation.
