The galaxy presents a largely smooth, elliptical morphology. Its light profile is centrally concentrated with a gradual decline in intensity moving outwards. The core region exhibits a bright, yellowish-orange hue, suggesting a dominant population of older stars. There are no clear indications of spiral arms or significant dust lanes. The galaxy appears relatively undisturbed, with no strong evidence of recent major mergers or tidal features. The overall color suggests it is a relatively quiescent galaxy with suppressed star formation, dominated by an older stellar population.
