The galaxy presents as a largely smooth, elliptical or lenticular morphology, exhibiting a concentrated central bulge that dominates the overall light profile. The core region shows a strong yellowish-white emission, suggestive of a population of older stars. The outer regions fade gradually into the background sky, showing a subtle color gradient, from the yellow core to a more reddish halo. There is no obvious indication of strong spiral arm structure or significant dust lanes. There may be a minor disturbance in the form of some asymmetric features, but this is difficult to determine. Overall, it looks like an older, relatively quiescent galaxy.
