The galaxy presents as an elongated, disk-shaped structure, oriented almost perfectly edge-on with respect to our line of sight. The central region exhibits a higher surface brightness, suggestive of a galactic bulge. There is a noticeable absence of spiral arm structure, and the disk appears smooth and relatively featureless. Some bluer colors are visible along the disk. The galaxy shows no obvious signs of a major merger or significant tidal disturbances, and the bulge appears relatively normal. The disk is very thin and well defined, suggesting a stable and relaxed morphology.
