The galaxy presents a largely smooth, elliptical morphology. The central bulge exhibits a concentrated, bright yellow-orange hue, suggesting a significant population of older stars. There is a subtle, though discernable, gradation in color and brightness extending outward from the core. The outer regions appear less luminous and exhibit a slightly bluer tint compared to the central bulge, possibly indicating the presence of younger stellar populations or a lower concentration of dust. There is no indication of prominent spiral arms or a distinct disk structure. There are no obvious signs of ongoing major mergers or significant tidal disturbances. A faint, diffuse halo surrounds the main body of the galaxy, although its exact boundaries are difficult to discern. Overall, the galaxy appears to be a relatively evolved system.
