The galaxy presents a smooth, elliptical morphology. It appears to be relatively round, displaying a gradual decrease in luminosity from its core outwards. The core exhibits a reddish-orange hue, likely indicating an older stellar population. The outer regions show a faint transition to a slightly bluer color, possibly due to the presence of younger stars, although this is minimal. There's no strong evidence of prominent spiral arms or significant dust lanes. Overall, the galaxy seems to be a fairly undisturbed, evolved system with a low star formation rate. No clear signs of ongoing mergers or major disturbances are apparent.
