The galaxy presents as a relatively compact, elliptical-like structure with an overall smooth appearance. A slight elongation is observed, deviating from a perfectly circular morphology, suggesting a possible prolate spheroidal shape. The luminosity distribution is centrally concentrated, with a gradual decrease in brightness towards the outer regions. There is a distinct color gradient, with a redder core region transitioning to bluer outer regions. There is evidence of a possible tidal interaction or ongoing merger event as seen in the overall disruption of the galaxy shape.
