The galaxy presents as a relatively smooth, elliptical morphology. It appears to be quite luminous, exhibiting a pronounced central bulge with a gradual decrease in luminosity towards its outer regions. The color profile indicates a dominance of older stellar populations, likely composed of low-mass stars, as evidenced by its reddish-yellow hue, while the outer edges may contain a small amount of younger stars which is shown in the greenish hue around the yellow middle. The overall structure suggests it is undisturbed, lacking prominent tidal features or signs of recent mergers. The observed shape appears close to spherical.
