The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge, with a color gradient suggesting a population of older stars dominating the core. The outer regions appear more diffuse, potentially indicating a transition to a less densely populated stellar halo. There's little evidence of significant disk structure or spiral arms. The overall color is moderately red, implying a relatively passive star formation history with a low rate of current star formation. No signs of major mergers or tidal disturbances are apparent, suggesting a relatively isolated and stable system. There is a slight deviation from perfect circularity but this is minimal.
