The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a strong concentration of yellow light, suggesting an older stellar population dominating the core. Moving outward from the center, the light becomes more diffuse and redder in hue. There is little evidence of spiral arms or significant dust lanes. The overall structure appears regular, with no obvious signs of ongoing major mergers or tidal distortions. The light profile suggests a galaxy that is relatively undisturbed, having reached a stable morphological configuration.&#x20;
