The galaxy presents as a fairly smooth, elliptical-like structure. There is a concentrated central bulge with a gradual decrease in luminosity extending outwards. The color appears predominantly yellow, suggesting an older stellar population and relatively low ongoing star formation. There are no visible spiral arms or dust lanes. The galaxy is relatively compact, with a somewhat round, relaxed morphology. There is no evidence of any major merger activity, such as tidal tails or disturbed morphology, but there is a very slight chance of a minor disturbance in the galaxy shape.
