The galaxy presents a largely smooth, elliptical morphology, appearing as a concentrated central bulge with a gradual decrease in luminosity towards the outer regions. There is no apparent spiral structure or distinct features such as prominent dust lanes or star-forming regions. The color profile suggests a more evolved stellar population, displaying a reddish-yellow hue indicative of older, cooler stars dominating the galaxy's light output. The galaxy is moderately sized with a well defined shape. There is no evidence of ongoing major mergers or significant tidal disturbances.
