The galaxy appears as a centrally concentrated object with a smooth overall morphology. The central region exhibits a yellowish-white hue, suggestive of an older stellar population. Moving outwards from the core, there's a subtle shift towards a more greenish-blue color in the outer regions, potentially indicating the presence of younger, hotter stars. There are no clear signs of spiral arms or a prominent disk structure. The galaxy appears relatively undisturbed, without any significant tidal features or signs of ongoing mergers.
