The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated brightness profile, with the intensity diminishing gradually towards the outer regions. The overall shape is more round than elongated. The galaxy appears to have a primarily homogenous color, with a slight reddish hue, that suggests an older stellar population and little ongoing star formation. There is some indication of potential disturbances within the galaxy. The structure is not perfectly uniform, showing minor asymmetries or irregularities that might be indicative of tidal interactions or recent mergers.
