The galaxy presents a generally elliptical morphology, although subtle irregularities are apparent in its structure. The central region exhibits a bright, concentrated luminosity, indicative of a substantial stellar population. The overall color gradient suggests an older stellar population dominating the central bulge, with a shift towards slightly bluer hues in the outer regions. A hint of disk-like structure is possibly present. The galaxy appears to be undergoing some form of interaction, as evidenced by the asymmetry and possible tidal features. The observed characteristics suggest a relatively massive galaxy with ongoing, albeit potentially quiescent, star formation.
