This galaxy presents as an edge-on spiral, exhibiting a disk-like structure with an apparent major axis. The disk appears relatively smooth and elongated. A bulge is visible, appearing rounded rather than boxy. There's a subtle color gradient across the disk, suggestive of differing stellar populations or dust distribution. No strong signs of recent major mergers or significant tidal disturbances are observed, although minor disturbances can not be ruled out. The galaxy's apparent size suggests it is a moderate-sized galaxy at a cosmological distance, with an appreciable star formation rate.
