The galaxy appears to be a relatively smooth, centrally concentrated system. The light profile suggests an elliptical morphology, although some subtle disk-like structure cannot be ruled out. The galaxy exhibits a bright, compact core that diffuses outwards. There's a slight blue tinge in the outer regions, potentially indicating some ongoing star formation, although it is not overtly active. There is a faint, asymmetric extension or tidal feature visible on one side, suggestive of a minor interaction or past merger event. This could also explain the disk-like structure. Overall, the galaxy seems to be an intermediate mass object at a moderate redshift.
