The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The light distribution suggests a dominant older stellar population, giving it a yellowish-orange hue. There is little evidence of spiral arms or significant dust lanes. Faint, irregular extensions surround the central region, suggestive of possible tidal interactions or recent minor merger events. A slightly brighter, more diffuse region appears offset from the primary nucleus. The galaxy exhibits a somewhat rounded shape but not perfectly spherical. 
