The galaxy presents as a largely featureless, elliptical morphology. It exhibits a smooth, centrally concentrated luminosity profile, appearing nearly spheroidal in shape, though with a subtle elongation along one axis. The color gradient suggests a concentration of older stellar populations towards the galactic center, as evidenced by the yellowish-white hue, which gradually fades into a bluer tint in the outer regions. There is no discernible dust lane or spiral arm structure visible. Overall, the galaxy gives the impression of a relatively relaxed system, likely dominated by evolved stars and possessing a substantial mass. There may be some minor asymmetry or disturbance present, but it is difficult to determine the cause with the available data.
