The galaxy presents as a somewhat diffuse, elliptical-like structure. There appears to be a noticeable color gradient within the galaxy. The central region exhibits a more yellowish-orange hue, suggestive of an older stellar population and/or significant dust obscuration. Moving outward from the center, the galaxy transitions to a bluer tint, potentially indicative of younger, hotter stars. The overall morphology appears relatively smooth and undisturbed, showing little evidence of spiral arms or irregular features. There appears to be two distinct blobs of differing colors indicating this may be an ongoing or recently completed galactic merger.
