The galaxy presents a flattened, disk-like morphology, consistent with a spiral or lenticular classification. The central region exhibits a bright, yellowish-white hue, suggesting a population of older stars and/or significant dust obscuration. Moving outwards, the disk displays a bluer tint, potentially indicative of ongoing star formation within spiral arms or a younger stellar population. The overall shape appears elongated, with a distinct major axis and a relatively narrow minor axis. The galaxy appears relatively undisturbed, showing no strong signs of a recent major merger event. The outer regions fade into the background, with no clearly defined edge to the galactic disk.
