The galaxy exhibits a generally smooth, elliptical morphology with a centrally concentrated bulge. The color profile transitions from a yellowish-white core to a bluer halo, suggesting a population shift from older stars in the center to younger, possibly star-forming regions in the outer parts of the galaxy. There is no strong evidence of spiral arms or a distinct disk structure. The galaxy appears relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions. However, there may be some minor asymmetry visible, potentially hinting at a subtle past interaction or internal activity. The lack of prominent dust lanes suggests the galaxy is relatively evolved.
