The galaxy presents a largely smooth, elliptical morphology. There is a concentrated central bulge, with a gradual decrease in luminosity extending outwards. The color appears relatively uniform across the galaxy, shifting from a yellow core to a reddish outer halo. No prominent dust lanes, spiral arms, or distinct features are visible. The smooth, centrally concentrated light distribution suggests that this is a relatively old galaxy with little ongoing star formation, or perhaps only limited activity in the inner regions, in comparison to its mass. There is no evidence of interactions or major disturbances in its shape.
