The galaxy presents as a fairly smooth, elliptical morphology. The central bulge exhibits a bright, concentrated luminosity gradient, indicating a high stellar density, likely composed of older stellar populations. The outer regions display a gradual decrease in surface brightness, transitioning to a fainter, more diffuse halo. There is a slight elongation evident in the overall shape, deviating marginally from a perfectly circular form. Subtle color variations are discernible, with a generally yellower hue in the core region, potentially indicative of older stars. Fainter blueish regions are visible in what appear to be faint extended disk features, suggesting ongoing, though relatively subdued, star formation activity. There is no evidence of major mergers or significant tidal disturbances in this image, with no strong signs of interacting companion galaxies or distorted morphology.
