The galaxy presents as an elongated, likely spiral galaxy, viewed edge-on. A central bulge is visible, appearing yellowish-orange, suggestive of an older stellar population. Moving outward from the bulge along the galactic plane, the disk exhibits a blue hue, possibly indicative of ongoing star formation within the spiral arms. The galaxy has a disk-like structure without any signs of mergers or major disturbances. The outer edges appear slightly fuzzy, which could be due to faint, unresolved spiral arms or dust. The galaxy's overall morphology appears relatively smooth and undisturbed.
