The galaxy presents as a relatively smooth, centrally concentrated object. There is a slight elongation, deviating from a perfectly circular form. A dominant, bright central region is apparent, potentially indicative of a prominent galactic nucleus. Surrounding the core, a more diffuse, fainter halo of light extends outwards. There's a subtle color gradient, with the central regions appearing slightly more reddish-orange, possibly indicating an older stellar population. The outer halo exhibits a bluer hue, suggesting the presence of younger, hotter stars. The overall morphology doesn't show any signs of major disturbances or ongoing mergers, although some minor irregularities or extensions cannot be entirely ruled out.
