The galaxy presents as a generally smooth, elliptical morphology. The central region exhibits a high degree of luminosity, appearing bright and concentrated. The light emanating from this central area graduates outwards into a slightly more diffuse halo, indicating a gradual decrease in stellar density. There's a subtle color gradient, shifting from a warmer, yellowish hue in the core to slightly cooler tones towards the outer edges of the galaxy. This could be indicative of differing stellar populations or dust distribution. There's no immediately apparent spiral structure, and the galaxy appears largely undisturbed, exhibiting no major signs of ongoing mergers or significant tidal disruptions. The overall structure suggests an evolved system.
