The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that is more yellow in color, suggesting an older stellar population and minimal recent star formation. Surrounding the central region is a more diffuse halo or disk-like component. This outer region is bluer than the core, indicating the presence of younger, hotter stars, and potentially ongoing star formation, albeit at a low rate. The overall shape suggests a galaxy that is somewhere between being perfectly round and cigar-shaped. There is no immediately obvious sign of strong tidal interactions or major mergers occurring, but the slightly irregular shape could indicate minor disturbances or past interactions. The galaxy is of intermediate size and luminosity, suggesting a moderate stellar mass content.
