The galaxy presents as a centrally concentrated object with a smooth light profile. The core exhibits a yellowish-white hue, suggestive of an older stellar population. Moving outwards from the core, the color shifts to a slightly redder shade. The shape appears to be more elliptical than circular, indicating a moderate degree of flattening. There is no discernible evidence of spiral arms or a prominent disk structure. The galaxy appears relatively undisturbed, with no obvious signs of ongoing mergers or tidal interactions.
