The galaxy presents a largely smooth and rounded appearance. The central region exhibits a yellowish-white color, suggesting a concentration of older stars. The outer regions show a slightly bluer hue, potentially indicative of ongoing, albeit subdued, star formation. There is no strong evidence of spiral arm structure or a prominent disk component. The galaxy appears undisturbed, without any signs of tidal tails or major morphological distortions suggestive of recent mergers. Overall, the morphology aligns with that of an elliptical galaxy, although a very faint disk component cannot be ruled out given the image resolution.
