This galaxy appears to be a spiral galaxy, oriented edge-on from our perspective. There is a notable central bulge that appears bright and somewhat rounded. The disk is clearly visible, extending outward from the bulge, and appears relatively smooth. No spiral arm structures are apparent, most likely due to the viewing angle. The galaxy exhibits a color gradient, with the bulge appearing more yellow/white, suggesting an older stellar population, and the disk a slightly bluer tint, which suggests the potential for ongoing star formation. There is no evidence of significant dust lanes or major disturbances in the disk. The general morphology suggests a well-formed, relatively undisturbed spiral galaxy.
