The galaxy appears to be elliptical in morphology, with a high degree of central concentration. The light distribution is relatively smooth, with a noticeable lack of spiral arm structure or prominent dust lanes. There may be a slight indication of tidal disturbances, but it is very subtle. The galaxy is moderately bright and compact. The shape is mostly round but not perfectly spherical, and does not look disc-like. There may be a slight hint of asymmetry in the outer regions, which could be due to a minor past or ongoing interaction, although the overall morphology indicates a non-merging system.
