The galaxy presents as a generally smooth object, appearing elliptical in shape. It exhibits a concentrated central bulge with a gradual decrease in luminosity toward the outer edges. The color profile indicates a population of older stars, with a slightly redder hue dominating the overall appearance. There is no apparent spiral structure, and the lack of significant blue coloration suggests minimal ongoing star formation within the observable bands. Minor irregularities in the outer regions indicate possible gravitational interactions or past mergers, though the overall structure remains largely undisturbed. The galaxy does not show evidence of a strong tidal tail or bridge, indicating a potentially stable and relaxed system.
