The galaxy presents as a relatively smooth, centrally concentrated object with a somewhat elliptical morphology. The light distribution suggests a possible bulge component dominating the galaxy's structure. There is a slight asymmetry in the outer regions, with subtle indications of possible tidal features or minor disturbances. Faint, diffuse light extends outwards from the main body of the galaxy, indicating a stellar halo or envelope. There are no clearly defined spiral arms or prominent dust lanes visible within the galaxy, suggesting a lack of significant ongoing star formation or a more evolved stellar population. The overall color appears relatively red, consistent with a population of older stars. There is some indication of a faint, bluer region at the center, hinting at possible low-level star formation in the core. Overall, it appears to be an elliptical galaxy undergoing some form of interaction.
