The galaxy presents a largely smooth, elliptical morphology. Its light profile suggests a centrally concentrated structure with a gradual decrease in luminosity outward. The core region exhibits a bright, yellowish-white hue, potentially indicating an older stellar population. Moving outward from the center, the light fades into a diffuse, reddish-tinged halo. The overall shape is somewhat rounded, although a slight elongation is perceptible, possibly signaling a transition between a perfectly spherical and a more flattened ellipsoidal form. There are no distinct features such as spiral arms, bars, or dust lanes visible in the image. There are no signs of ongoing mergers or major disturbances. The galaxy appears relatively undisturbed and in a settled state. The apparent angular size is small, suggesting a relatively distant object.
