The galaxy presents as a moderately bright, fairly smooth elliptical-like structure. There is a bright central bulge with a diffuse, extended halo. There may be a slight asymmetry or faint arm-like feature on the galaxy's periphery which could be a sign of a minor disturbance or interaction. The overall color appears to be on the redder side, possibly indicating an older stellar population and/or a relatively low rate of star formation. The morphology suggests that it could be a relatively massive galaxy.
