The galaxy presents as a relatively smooth, elliptical-like structure. It appears highly concentrated with a bright central region, suggesting a significant bulge component. No distinct spiral arms or prominent dust lanes are visible. The galaxy exhibits a generally round shape. There are slight indications of some disturbances, which may suggest minor interactions with other galaxies or recent internal activity. The color profile indicates a population of older stars. Overall, the galaxy appears to be a massive, evolved system.
