The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a high degree of luminosity, appearing bright and concentrated. Moving outward from the core, the light gradually diminishes, creating a diffuse halo. There is a faint hint of a disk-like structure, although it is not clearly defined. The overall color of the galaxy seems slightly redder in the central regions, transitioning to bluer hues in the outer parts. The image shows no major signs of ongoing mergers or significant tidal disturbances, suggesting that the galaxy is relatively undisturbed. There are hints of some features and substructure within the extended halo. The galaxy's shape is elongated, with a ratio of major to minor axis close to but less than 2:1, displaying a mostly elliptical profile.
