The galaxy presents a generally smooth, elliptical morphology, appearing mostly featureless. The central region exhibits a concentrated luminosity, appearing brighter than the outer regions. The radial profile suggests a gradual decrease in brightness from the center outwards. A slight elongation is observed, but it is not markedly cigar-shaped. The color indices suggest a population of older stars; the dominant colors are indicative of intermediate age stars. There are no obvious signs of ongoing major mergers or significant tidal disturbances. The galaxy appears to be relatively undisturbed.
