The galaxy appears as a centrally concentrated, luminous object with an elliptical morphology. The core region exhibits a bright, yellowish-white hue, suggesting a population of older stars. The light gradually fades outward, transitioning to a more diffuse, reddish-orange halo. The structure shows no distinct spiral arms or significant dust lanes, leading to a generally smooth appearance. There is a slight elongation of the galaxy along its major axis, although it appears substantially round. Faint extensions of light can be observed, indicating possible tidal features or a more extended stellar halo, although their definition is limited. There are no apparent signs of active merging or major disturbances in its structure. Overall, the galaxy presents characteristics consistent with a massive, evolved elliptical galaxy at a considerable distance.
