The galaxy presents an elliptical morphology, appearing largely smooth in texture, with a subtle elongation. Its color profile is predominantly yellowish-orange, suggesting a stellar population that is primarily composed of older stars. There is little evidence of distinct spiral arms or significant dust lanes. The galaxy’s core appears to be brighter and more concentrated than its outer regions, with a gradual decrease in luminosity towards the periphery. Faint extensions appear along the major axis of the galaxy, indicating possible tidal interactions. The overall structure suggests a relatively evolved system.
