This galaxy appears as a fairly smooth, elliptical-like object. It presents a concentrated central bulge that gradually diffuses outwards. The overall color is predominantly reddish, suggesting an older stellar population. There is some evidence of a slight disk-like structure, though it is not sharply defined. A faint blue tinge can be seen in some of the galaxy's outer regions, potentially indicating regions of localized recent star formation. There is evidence of some gravitational disturbance and a merger in progress, with the main body of the galaxy appearing somewhat disrupted and displaying possible tidal features or an interacting secondary object in its vicinity. The majority of the light appears to be centrally condensed, hinting at an older, more evolved system with a high mass concentration.
