The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a yellowish hue, suggesting a population of older stars. The outer regions display a gradual decrease in surface brightness, appearing more diffuse and with a slightly bluer tint. This bluer color indicates the presence of younger, hotter stars in the outer regions.

There is a slight asymmetry and subtle disturbance in the galactic disk, possibly due to a past interaction. Overall, the galaxy appears relatively undisturbed with no prominent tidal features or signs of a major ongoing merger.
