The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. It displays a gradual decrease in luminosity from the core outwards, lacking distinct spiral arms or a prominent disk structure. The galaxy exhibits a yellowish-white hue in its central region, suggestive of an older stellar population. A faint, diffuse halo surrounds the core, extending further out with a bluer color gradient, possibly indicating the presence of younger stars or recent star formation activity in the outer regions. The galaxy appears relatively undisturbed, showing no signs of major mergers or tidal disruptions. There is some evidence of minor disturbances or irregular features in the outer halo, but overall the structure is largely smooth and symmetrical. The object is approximately round but elongated.
