The galaxy presents an elliptical morphology, appearing mostly smooth with a slight elongation. The color gradient indicates a redder core, likely composed of an older stellar population, with bluer outer regions suggestive of ongoing or recent star formation. There is a hint of a disk-like structure present in the galaxy. The overall structure is relatively undisturbed, without any obvious signs of major mergers, though some minor tidal features might be present. It is likely a massive galaxy with a low star formation rate.
