The galaxy appears as a relatively smooth, centrally concentrated elliptical or lenticular galaxy. There is little to no indication of spiral arm structure. The galaxy exhibits a near-spherical shape, with only a slight deviation towards a more elliptical form. No obvious signs of tidal disturbances, major mergers, or significant morphological peculiarities are visible. The galaxy exhibits a notable red color, indicating a stellar population dominated by older stars with minimal ongoing star formation.
