The galaxy appears to be a relatively smooth, elliptical type. It exhibits a bright, concentrated central bulge that dominates its overall structure. There appears to be some distortion in its shape, possibly due to a tidal interaction. The galaxy displays a color gradient, transitioning from a bluer core region to redder outer regions, suggesting a variation in stellar population age across its extent. One of the sides appears to have a long tail, implying a merger with a satellite galaxy. There is no noticeable spiral structure. Overall, the object has a smooth appearance with indications of a recent interaction and relatively active star formation.
