The galaxy appears as a relatively smooth and rounded elliptical galaxy. There is a distinct lack of discernible spiral arm structure or strong dust lane features within the galaxy's body. The light distribution appears centrally concentrated, decreasing gradually towards the outer regions of the galaxy. There is a minor, somewhat irregular feature possibly indicating some tidal interaction or minor disturbance in morphology. The galaxy exhibits a redder color profile. This points towards an older stellar population, and lower levels of recent star formation activity. It exhibits significant mass in the central regions, and a relatively high mass overall.
