The galaxy presents as a fairly smooth, elliptical-like structure. It exhibits a bright, concentrated central region, suggesting a prominent galactic nucleus. The morphology appears predominantly spheroidal with a notable lack of distinct spiral arm features. The color gradient transitions from a yellow-white core to a slightly redder halo, potentially indicating an older stellar population dominating the galaxy's composition. There is a marginal hint of a disk, with a very small blue edge. A faint, diffuse halo surrounds the galaxy, but there is no readily apparent dust lane or significant morphological disturbance, thus indicating it is not undergoing major merging or strong interactions.
