The galaxy presents as a relatively smooth, centrally concentrated object with an elliptical morphology. It exhibits a predominantly yellowish hue in its central region, suggestive of an older stellar population. A slightly more reddish component is visible, offset from the center, potentially indicative of ongoing, albeit subdued, star formation or dust obscuration. There are no discernible spiral arms or significant dust lanes. Overall, the galaxy appears relatively undisturbed, showing no obvious signs of major mergers or tidal interactions. It appears nearly round.
