The galaxy presents as a flattened, elongated structure, indicative of a disk galaxy viewed at a steep inclination, approaching edge-on. The central bulge appears relatively small and concentrated, exhibiting a yellowish hue. The disk component shows a bluer tint, suggesting the presence of younger stellar populations. The galaxy appears relatively smooth and the bulge is small compared to the rest of the galaxy. The outer regions of the disk fade gradually, with no distinct breaks or rings visible. There are no immediately obvious signs of significant dust lanes or strong star-forming regions resolved in the disk, though the blue color suggests ongoing star formation is present.
