The galaxy presents a largely smooth and rounded morphology. It exhibits a concentrated central bulge with a diffuse halo extending outwards. The galaxy's color profile indicates a dominant population of older stars, likely resulting in a redder appearance. There are no readily apparent spiral arm structures or significant dust lanes visible in this image. No signs of tidal disturbances or active galactic nuclei are observable. This galaxy appears to be a relatively undisturbed, mature system.
