The observed galaxy presents a clear disk morphology, viewed nearly edge-on. The disk exhibits a noticeable warp or asymmetry, potentially indicative of past interactions or internal disturbances. A central bulge is present, though somewhat obscured by the edge-on perspective. There is a prominent dust lane visible along the mid-plane of the disk, attenuating light from the bulge and further disk regions behind it. The disk itself appears relatively smooth, but with hints of spiral arm structure faintly visible. Star formation appears to be concentrated in the disk, as evidenced by the bluer colors and localized bright spots. The overall color suggests a galaxy with ongoing star formation, with the dust lane and morphology pointing towards a spiral classification. No obvious signs of a major merger are apparent, but there may be minor tidal features hinting at a possible interaction with a smaller galaxy.
