The galaxy appears to be a relatively compact, elliptical system. It exhibits a smooth, centrally concentrated light profile with no discernible spiral arms or disk features. The morphology suggests an older stellar population, although there is a subtle blueish tint at the core, potentially indicating a small amount of ongoing star formation. The isophotes appear close to round and there are no obvious signs of tidal interactions or major disturbances. There are no significant signs of a galactic merger, such as distorted shapes or double nuclei.
