The galaxy presents a largely smooth, elliptical morphology with a centrally concentrated bulge. There is some indication of a disk component, although this is subtle. The galaxy exhibits a color gradient, transitioning from a bluer hue in the central regions to a redder hue in the outer regions, potentially indicative of older stellar populations in the outskirts. The galaxy's structure appears relatively undisturbed, with no obvious signs of recent major mergers. There is the possibility of minor interactions or disturbances in the vicinity. Star formation is likely ongoing, albeit at a moderate rate, given the relatively blue color of the central region.
