The galaxy appears to be a relatively smooth, elliptical or spheroidal galaxy, with a high degree of central concentration. There is little evidence of spiral arm structure or significant dust lanes. The light profile suggests a centrally concentrated bulge with a fairly uniform decrease in intensity outwards, consistent with an early-type morphology. The galaxy exhibits a yellowish-orange hue, which implies an older stellar population, and diminished star formation activity. There are no obvious signs of a major ongoing merger or significant tidal distortions, though there might be some minor disturbance. It exhibits a rounded shape with a high degree of circularity.
