The galaxy appears to be a relatively smooth object, likely an elliptical, although some features are apparent. The central region exhibits a concentrated luminosity gradient, appearing quite bright and potentially yellowish or golden in color. There is an elongation or tail feature extending outwards from the central region, which might be indicative of tidal interactions or ongoing merging activity. This feature has a bluish tint, suggesting the presence of younger, hotter stars. The galaxy has a generally rounded shape, with some deviation from perfect circularity, potentially influenced by interactions or internal dynamics. Overall the galaxy seems relatively old and massive with low star formation. 
