This galaxy presents as an edge-on spiral with a disk-like structure dominating its overall form. The central bulge appears prominent and shows a slightly rounded morphology. The disk exhibits a notable warp or bend along its primary axis, suggestive of gravitational interaction or past merger events. Evidence of potential tidal features or disrupted structures extends outward from the main galactic body on one side. The color distribution suggests an older stellar population in the bulge, with bluer hues visible along the disk, possibly indicating regions of active star formation. There appears to be a minor dust lane visible near the central bulge.