The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. The central region is significantly brighter and appears yellow-white, indicative of a population of older stars. The outer regions exhibit a fainter, more diffuse halo. The galaxy appears largely undisturbed, showing no obvious signs of major mergers or tidal interactions. The shape is generally elliptical, exhibiting a slight deviation from perfect circularity, appearing somewhat elongated along one axis. There may be a slight indication of a disk structure in the outer regions, but the overall appearance is dominated by the spheroid. There is little evidence of ongoing star formation or prominent spiral arm structures.
