The galaxy appears as a slender, edge-on spiral, with a notable central bulge and a thin disk extending outwards. The bulge presents a smooth, relatively featureless profile in contrast to the disk. Dust lanes are clearly visible within the disk, appearing as dark, obscuring bands that run along the galactic plane. There is evidence of some star formation as seen by the subtle blue hue within the galactic disk. The structure appears relatively undisturbed with no signs of a major merger event. There appears to be minor irregularities in the disk, suggesting mild gravitational disturbances.
