The galaxy appears as a relatively compact, elliptical-shaped object. Its light profile appears smooth with a high degree of central concentration and no obvious substructure such as spiral arms or a bar. The galaxy displays a uniform color, with no distinct regions of intense star formation evident. The overall color is consistent with an older stellar population. The isophotes are relatively regular, with a slight deviation from perfect circularity. There is no indication of tidal tails or other signs of recent major merger activity.
