The galaxy presents as a largely smooth, elliptical-like structure with a centrally concentrated light profile. The color appears relatively uniform, with a slight tendency towards redder hues, particularly at the core, suggesting a population of older stars. There are no readily discernible spiral arms or significant dust lanes. The galaxy exhibits a high degree of circular symmetry. There are no obvious signs of recent or ongoing major merger events. Subtle irregularities in the outer regions may suggest minor gravitational interactions or past accretion events. Overall, the galaxy appears to be a mature system, potentially a massive elliptical galaxy with a relatively quiescent star formation history.
