The galaxy presents as a relatively smooth, centrally concentrated object, likely an early-type galaxy. It exhibits a roughly elliptical morphology, appearing largely rounded with minimal elongation. There is no clear evidence of spiral arms or a distinct disk structure, and no apparent major disturbances or tidal features that would indicate ongoing or recent merger activity, although there is some indication of minor disturbance. The galaxy displays a color gradient, transitioning from a more yellow/orange core region outward to a fainter and slightly bluer halo, suggesting a radial difference in stellar populations, with older populations dominating the core. Overall, the galaxy appears to be a fairly massive system with a moderate rate of star formation.
