The galaxy presents a largely smooth and rounded morphology, lacking prominent spiral arms or a defined disk structure. The light is concentrated towards the central region, suggesting a high stellar density or the presence of a bulge. Faint extensions or minor disturbances might be present, suggesting the possibility of past minor interactions with other galaxies, though no obvious signs of active merging are visible. The color gradient across the galaxy indicates a possible variation in stellar populations, with the central regions appearing yellower, potentially indicative of older, redder stars, and outer regions with a bluish tint, possibly indicative of younger, bluer stars.
