The galaxy presents as a relatively smooth, centrally concentrated elliptical galaxy with a high degree of circular symmetry. The core exhibits a bright, yellowish hue, indicative of an older stellar population likely dominated by red giant and dwarf stars. A subtle blue halo surrounds the central region, suggesting the presence of a younger, though less prominent, population of stars. No distinct spiral arms or significant dust lanes are apparent. There are no signs of ongoing major mergers or tidal disturbances. Based on the morphology, the galaxy appears to be relatively undisturbed and evolved.
