This galaxy presents a disk-like morphology, observed nearly edge-on from our vantage point. A prominent central bulge, characterized by a yellowish hue, is visible. The disk component exhibits a bluer color gradient towards its outer edges, suggestive of ongoing star formation within the spiral arms. Some asymmetry is present within the disk, indicating the presence of minor disturbances. There may be faint tidal features that further suggest an interaction. Dust lanes appear present along the equatorial plane obscuring the central bulge. The overall structure of the galaxy suggests a late-type spiral. 
