The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The light distribution appears centrally condensed, with a gradual decrease in luminosity moving outwards from the core. It exhibits a predominantly yellowish-orange color, indicative of an older stellar population. There is no discernible spiral structure or prominent dust lanes visible. The galaxy appears fairly isolated, showing no significant tidal distortions or indications of recent mergers, although there are a couple of fainter objects nearby. The overall morphology suggests a system dominated by evolved stars with a relatively low rate of ongoing star formation. The object displays a high degree of circular symmetry, implying a dynamically relaxed state.