The galaxy presents as a relatively smooth, centrally concentrated object. The overall color appears reddish, suggesting a population of older stars and a limited amount of ongoing star formation. The light distribution exhibits a mostly elliptical morphology, with a gradual decrease in luminosity from the core outwards. There is a subtle extension to the upper left, suggesting a potential minor interaction or tidal feature. The structure lacks distinct spiral arms or prominent dust lanes, hinting at a classification along the elliptical-lenticular sequence.
