This galaxy appears to be a relatively smooth, centrally concentrated object. The light is distributed in a roughly elliptical shape, with a higher concentration of yellow-orange light towards the center, which may indicate an older stellar population concentrated at the core. Fainter, slightly bluer light extends away from the center in a more diffuse halo. This bluer component could be indicative of ongoing, but low level, star formation. There is no strong evidence of spiral arms or a well-defined disk structure. The overall morphology suggests it is likely an elliptical galaxy or a lenticular galaxy viewed face-on. There are no readily apparent signs of major mergers or significant tidal disturbances, though subtle asymmetries could suggest minor interactions in the past.
