The galaxy presents as a relatively smooth, elliptical-like structure. Its core appears bright and concentrated, showing a gradual decrease in luminosity extending outwards. The morphology is dominated by a spheroidal component, with no discernible spiral arms or bar structure visible. The galaxy appears slightly elongated, not perfectly circular. There is no evidence of any major ongoing merger events or strong tidal disturbances. Subtle color variations can be observed, possibly indicating different stellar populations throughout the galaxy, although the resolution limits detailed analysis. The overall form suggests a system that has largely completed its merging history and is in a relatively quiescent state.
