The galaxy presents as a largely smooth, elliptical structure. It exhibits a concentrated, bright central bulge that diffuses outward into a less luminous halo. There is no readily apparent disk component or spiral arm structure. The color profile suggests a population of older stars, trending toward redder wavelengths. The overall morphology appears undisturbed, showing no evidence of recent major mergers or significant tidal interactions with neighboring galaxies. The high degree of smoothness implies it is a well-mixed, evolved system.
