The galaxy appears to be elliptical in morphology, with a smooth and nearly round profile. The central region exhibits a strong concentration of light, indicating a dense stellar population. A gradual decrease in luminosity is observed moving outward from the core, with the outer regions fading into the background. There is a subtle color gradient from the center outward; the core displays a yellowish-orange hue, suggesting older stellar populations. The galaxy shows no apparent spiral arm structure or significant dust lanes and exhibits no visible signs of ongoing major mergers or tidal disturbances. Overall, the galaxy is generally quite round in shape.
