This galaxy presents a largely smooth and centralized morphology. It appears elliptical in shape, with the major axis slightly more extended than the minor axis. The light distribution is concentrated towards the center, suggesting a prominent bulge. There's a gradual falloff in luminosity from the core outwards, with no readily discernible spiral arm structure or significant dust lanes. There might be some subtle features present in the outer regions that could indicate minor disturbances, potentially from a past interaction or merger event, though nothing major is clearly visible. The galaxy's color appears relatively uniform across its extent, likely indicating an older stellar population and subdued star formation activity.
