The galaxy presents as a somewhat elliptical structure with a smooth overall appearance. The central region exhibits a concentrated luminosity, appearing yellowish-white, suggesting a population of older stars. The light gradually diminishes outward from the core, transitioning to a slightly bluer hue in the outer regions, possibly indicating the presence of younger stellar populations within the galactic disk. The object does not show any obvious spiral arm structures or significant dust lane features. The general shape is moderately elongated, not perfectly spherical but also not extremely flattened. There's no strong evidence of major tidal disturbances or ongoing mergers visible in this image. It seems to be a relatively undisturbed system, with a centrally concentrated morphology.
