This galaxy presents as a centrally concentrated, relatively smooth object. The light distribution indicates an elliptical morphology. Its color profile is somewhat redder, particularly towards the core, suggestive of an older stellar population dominating the galaxy's composition. There's a subtle color gradient from the core to the outskirts, which may indicate a change in metallicity or stellar population. The overall appearance suggests a lack of significant current star formation. There are a couple of slightly off center blue spots which likely indicate areas of weak star formation. There is no evidence of significant tidal features, strong spiral arm structures, or ongoing mergers visible in this image.
