The galaxy appears to be an elliptical or lenticular galaxy, characterized by a smooth, relatively featureless light distribution. There is a bright central bulge that fades in intensity outwards. The overall shape is somewhat elongated. There is no evidence of spiral arms or significant dust lanes. Its color indices suggest a predominantly older stellar population. The light is heavily concentrated in the center. The galaxy shows a strong radial gradient in color, the inner region is more yellow-orange than the outskirts, which are redder. There is no sign of recent merger events.
