The galaxy presents as a singular, relatively concentrated object with a smooth morphology. The dominant coloration is a yellowish hue concentrated at its core, suggesting a population of older stars. Fainter, slightly bluer regions are observed extending outward from the core, possibly indicative of ongoing, albeit limited, star formation. The galaxy's shape is generally elliptical, appearing mostly round, with no readily apparent signs of spiral arms or a disk structure. There are no immediately obvious signs of ongoing mergers or major tidal disturbances, although subtle asymmetries in the outer regions cannot be ruled out definitively at this resolution. The object appears well-defined, with a relatively sharp gradient in luminosity from the center outwards.
