The galaxy presents as a centrally concentrated spheroid, exhibiting a smooth, featureless morphology. Its color profile suggests a relatively evolved stellar population, with a yellowish hue dominating the core region, indicative of older stars. The galaxy displays a high degree of circularity with only slight deviations. There is no evidence of significant tidal features or strong interactions with nearby galaxies, although subtle asymmetries might be present. The galaxy appears isolated, showing no clear signs of recent major merger activity, with the observed properties suggesting a galaxy that has largely completed its assembly. Overall, the galaxy appears to be a relatively relaxed system.
