The galaxy presents as a somewhat elliptical object, appearing relatively smooth with no immediately discernible spiral arm structure. Its light profile suggests a centrally concentrated bulge, with luminosity decreasing gradually towards the outer edges. The core appears bright and yellowish, implying a concentration of older stellar populations. Faint disturbances around the core indicate possible presence of galactic merger. The overall color is slightly reddish, potentially indicating a population of older stars and/or dust obscuration.
