The galaxy presents a largely smooth, elliptical morphology. There is no distinct spiral structure visible. It appears nearly spherical in shape, with only the slightest elongation discernible. The galaxy exhibits a bright, concentrated core region, which fades gradually towards the outer edges. The color profile suggests a greater concentration of older stellar populations, especially in the central bulge, as evidenced by its more yellow-orange hue. There appear to be no major disturbances or merger events ongoing, based on the lack of tidal tails or irregular features. Some minor asymmetry might be present, but the overall structure seems relatively undisturbed and quiescent.