The galaxy appears as a relatively faint, edge-on spiral. It exhibits a distinct, flattened disk structure. The bulge is not prominently defined, appearing as a slight central thickening within the disk. There is no apparent active galactic nucleus. The disk does not seem to have well-defined spiral arms, giving the impression of a smoother distribution of stellar populations throughout the plane of the galaxy. The light from the galaxy is largely consistent in color, ranging from slightly green/blue to white, with hints of redder regions near the center and extending outwards. Overall, the galaxy shows a morphology consistent with a relatively low-mass and low star-formation rate system. No major interactions with neighboring galaxies are visible. There might be some minor disturbances present, but nothing to the extreme of mergers. The galaxy is somewhat cigar-shaped.
