The galaxy presents as a relatively smooth, centrally concentrated object with an elliptical morphology. The light distribution suggests a high degree of symmetry and coherence. There is a lack of discernible spiral arm structures or prominent dust lanes. The color gradient indicates that the central region is yellower, which is consistent with an older stellar population. The outer regions appear slightly bluer, hinting at the presence of some younger stars, however, this is minor. The overall appearance indicates an evolved system, potentially an elliptical galaxy or a lenticular galaxy viewed nearly face-on. There is no indication of strong tidal interactions or recent merger events.
