The galaxy appears to be a spiral galaxy viewed at an oblique angle. There is a central bulge that is visibly yellow. The galaxy exhibits a disk structure, with one prominent arm visible. There is also a second faint arm that seems to extend from the central bulge in the opposite direction. The disk appears smooth and flocculent, without obvious strong spiral arm definition. There is a hint of some ongoing star formation activity within the spiral arm. The galaxy shows a distinct color gradient from the central regions, where the bulge appears more yellow, to the outer regions of the disk, which show some bluer regions, indicative of younger stellar populations.
