This galaxy exhibits a generally elliptical morphology, appearing relatively smooth in structure. The core presents a concentrated, bright region, suggesting a high stellar density. The light profile appears to fade gradually from the core outwards, with the outer regions appearing diffuse and less distinct. There is a slight asymmetry, but not indicative of a major merger event. The color index indicates a population of older stars. The object appears to be relatively massive with suppressed star formation. 
