The galaxy presents as a relatively smooth, elliptical-shaped object. There is a slight elongation noticeable but its roundness dominates its morphology. The primary color appears to be a yellowish-orange hue, suggesting an older stellar population. The lack of prominent blue regions or spiral arms indicates minimal ongoing star formation. Although the galaxy appears mostly undisturbed, there seems to be minor asymmetry in its structure, suggesting a possible past interaction or a small merger event. The galaxy displays a central concentration of light, hinting at a bulge component.
