The galaxy appears to be an edge-on spiral galaxy, possibly of type Sc. It exhibits a prominent, elongated bulge that is a yellowish-white hue, suggesting an older stellar population. A faint, diffuse disk extends outward from the bulge, with the disk being relatively smooth in appearance. There is a slight warp or asymmetry observed in the outer regions of the disk. No distinct spiral arm structure is discernible from this viewing angle. Dust lanes are present, obscuring some of the light from the bulge and the disk. The overall color suggests a galaxy that is actively forming stars, albeit at a modest rate. There is no clear evidence of a major merger event or significant tidal disruption, although some minor disturbances cannot be ruled out.
