The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The core region shows a bright, yellowish-white hue, indicating an older stellar population. Moving outwards from the core, the light gradually fades, transitioning to a bluer color in the outer regions, suggesting the presence of younger stars and possible ongoing star formation. There are no obvious spiral arm structures or significant dust lanes visible in this image. The overall shape appears relatively round, with a minimal deviation from circular symmetry. There are no obvious signs of a major merger, though some minor disturbances cannot be ruled out based solely on this image. The estimated size suggests that this galaxy is an intermediate sized system.
