The galaxy presents as a relatively large, edge-on spiral with a notable bulge component. The disk appears thin and elongated. The bulge exhibits a somewhat rounded morphology. There is some indication of dust lane obscuration along the mid-plane of the disk. Evident are what appear to be gravitational disturbances along the edge of the disk. A merging galaxy along the top of the disk is also observed. The galactic center appears orange, suggesting the presence of older stellar populations in the bulge. The disk appears slightly more blue, hinting at the presence of younger stars within the spiral arms, though these arms are not distinctly resolved. The galaxy is significantly redshifted.