The galaxy presents as a centrally concentrated, smooth object. It appears elliptical in shape, with a high degree of radial symmetry. The core region is noticeably brighter and exhibits a yellowish-white hue, suggesting a population of older stars. Moving outward from the core, the light becomes dimmer, transitioning to a reddish tinge. This indicates a subtle change in stellar populations, potentially with cooler, older stars dominating the outer regions. There may be very faint hints of a disk-like structure or very weak spiral arms, but the overall morphology is dominated by its smooth, centrally concentrated light profile, making it likely an elliptical or lenticular type galaxy. There is minimal indication of dust lanes or prominent star-forming regions. The colors and morphology point towards a galaxy that may be undergoing low levels of star formation. There also appears to be some minor disturbance in the outer halo of the galaxy.
