The galaxy appears as a moderately bright, disk-shaped structure. It exhibits a relatively smooth overall profile, with a slightly brighter central region, suggestive of a bulge. The color is predominantly blue-white, indicating a significant population of younger, hotter stars and potentially ongoing star formation. Faint, extended arms are possibly present, but the image resolution limits clear identification. Some minor irregularity might be present in the disk, possibly indicating some type of interaction or tidal feature, but its prominence is minimal. Overall, the galaxy presents as a relatively undisturbed spiral or lenticular system with moderate star-forming activity.
