The observed galaxy presents as a relatively small, centrally concentrated object. The core is very bright and dominates the overall appearance, exhibiting a bright blue-white hue indicative of potentially high stellar density and/or active galactic nucleus activity. A disk or ring-like structure appears to surround the bright core, displaying a mottled color gradient from blue-green nearest the center to subtle orange-red tones at the outer edge. The galaxy appears to be relatively undisturbed, with no obvious tidal tails or signs of a major merger event. However, there are slight irregularities in the shape of the disk, suggesting possible minor disturbances or interactions. Overall, the morphology suggests either a compact, actively star-forming spiral galaxy or a more amorphous early-type galaxy with ongoing central activity.
