The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high concentration of light, appearing almost uniformly bright and yellowish. There is a gradual decrease in luminosity towards the outer edges. The outer regions are less defined, with some faint, irregular extensions. No distinct spiral arms or prominent dust lanes are observed. Overall, the galaxy appears to be a mature system with little evidence of recent major mergers or significant ongoing star formation. It displays a somewhat round morphology with minor disturbances.
