The galaxy presents a largely smooth and elliptical morphology. Its core exhibits a concentrated luminosity, suggesting a significant stellar population. The overall color profile indicates a relatively mature system, with a redder hue dominating the central region and a slight blue tint on the edges, possibly indicating the presence of younger stars in the outer regions. No distinct spiral arm structures or significant dust lanes are visible. The galaxy appears undisturbed, exhibiting no obvious signs of tidal interactions or ongoing mergers. Its form is approximately round.
