The galaxy presents as a relatively compact object with a smooth, elliptical morphology. There is a slight elongation, but the galaxy is generally round in appearance. The light distribution is concentrated towards the center with a gradual decrease in intensity moving outward. There is a suggestion of some faint internal structure, possibly a very weak disk or some tidal features, but the overall impression is that of a system dominated by an older stellar population. The galaxy exhibits a color gradient, appearing slightly bluer towards the core than the outskirts, suggesting the potential presence of relatively recent star formation. However, it appears to be a fairly quiescent galaxy with a low star formation rate. There is no evidence of any strong ongoing mergers.
