The observed galaxy presents as an edge-on disk galaxy. A distinct dust lane bisects the galaxy's disk, obscuring light from the galactic plane. A bulge is visible, appearing largely smooth and rounded. The galaxy exhibits a subtle blue hue, suggestive of ongoing star formation, albeit at a subdued rate. No major morphological disturbances are apparent, indicating relative quiescence with no signs of recent major merger activity. The disk appears relatively thin, characteristic of stable disk galaxies. The galaxy's overall structure suggests it is a well-formed, undisturbed disk system undergoing normal evolutionary processes.
