This galaxy appears to be an elliptical galaxy. Its light profile exhibits a smooth, centrally concentrated distribution with a gradual falloff in intensity towards the outer regions. The galaxy is characterized by a nearly circular morphology. There are no visible signs of spiral arms or a prominent disk. A slight color gradient can be discerned, with the central regions appearing somewhat yellower than the outer edges. This suggests a population of older stars dominating the core region. The outer halo appears more blue, suggesting younger star formation might be present, albeit at a low rate. There is no clear indication of any ongoing major merging activity or significant tidal disturbances.
