The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The light is predominantly yellow/orange, suggesting an older stellar population with fewer young, hot stars. It exhibits a relatively high degree of roundness and no obvious signs of spiral arm structures. Faint, diffuse extensions surround the core region of the galaxy, potentially indicating a halo of older stars or tidal debris from past interactions. No distinct dust lanes or prominent star-forming regions are visible within the observed light. The overall structure appears relatively undisturbed, with a low probability of ongoing major merging activity, but the presence of some minor distortions cannot be ruled out.
