The galaxy presents as a luminous, elliptical morphology. The core appears bright and concentrated, with a gradual decrease in luminosity moving outward. There is evidence of a somewhat smooth structure, with no prominent spiral arms or bar features visible. A faint, diffuse halo surrounds the central region. The galaxy has a slightly round shape. There are no indications of major mergers or significant tidal disturbances in the immediate vicinity, but there is a hint of minor disturbances. The overall color profile suggests a population of older stars, but there also appears to be a hint of younger stars.
