The galaxy presents as a centrally concentrated, elliptical-like structure. It exhibits a smooth, diffuse light distribution with a high degree of central concentration and a decrease in surface brightness moving outward. The core region has a yellowish tinge, suggesting a population of older stars. The galaxy’s overall shape appears relatively round. No prominent spiral arms, bars, or significant dust lanes are discernible. No signs of tidal tails or strong morphological disturbances are evident, indicating the galaxy is likely not undergoing a major merger event. The light profile suggests a relatively quiescent galaxy, potentially with a low star formation rate.
