The galaxy appears to be an elliptical galaxy with a relatively smooth and spheroidal morphology. The light profile suggests a concentrated central bulge that diffuses outwards. The galaxy's core exhibits a yellowish hue, indicating an older stellar population likely dominated by red giants and low-mass stars. There is little evidence of spiral arm structure or prominent dust lanes. The outer regions of the galaxy appear fainter and more diffuse, with a slight color gradient, suggesting that star formation is more subdued in these areas. No tidal tails or other signs of recent or ongoing major mergers are readily apparent, though there might be evidence of minor disturbances. Overall, the galaxy presents a well-formed, relaxed structure, consistent with an evolved system that is past its peak star-forming activity.
