The galaxy presents as a relatively smooth, elongated structure indicative of an elliptical or lenticular morphology. The light distribution appears concentrated towards the center, with a gradual decrease in surface brightness moving outward. The color gradient suggests an older stellar population, with a yellowish-orange hue dominating the central region, potentially indicative of a larger population of older stars. There is a subtle bluer component towards the outer edges, possibly indicating some ongoing, albeit subdued, star formation. There are no obvious signs of spiral arms or significant dust lanes. The overall structure appears relatively undisturbed, without any major asymmetries or tidal features suggesting a recent major merger event. The galaxy exhibits a moderate redshift.
