The galaxy presents as a single, luminous structure with a smooth, centrally concentrated morphology. The core region exhibits a strong yellow hue, possibly indicative of an older stellar population. Moving outward from the core, the color transitions to a slightly cooler greenish-yellow. This could suggest a region with ongoing, but relatively low, star formation. The outer edges of the galaxy gradually fade into the background, displaying a faint blue-green tinge. The galaxy appears generally elliptical, with its width only slightly greater than its height. There are no distinct features visible such as spiral arms or prominent dust lanes; it appears largely undisturbed. There is no indication of tidal tails or major mergers.
