The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a concentrated, bright core, diminishing in intensity outwards. The galaxy appears nearly spherical in shape. There is no readily apparent evidence of spiral arms or a distinct disk structure. The color profile suggests a population of older stars, with a redder hue dominating the galactic body, particularly in the central bulge. There is no strong visual indication of ongoing major star formation activity or significant tidal disturbances. Subtle color variations might indicate some minor structural features, but the overall impression is that of a relaxed, relatively undisturbed system.
