The galaxy presents as an edge-on spiral, characterized by a prominent, flattened disk structure. Dust lanes are visible, obscuring some of the light from the galactic bulge and contributing to a mottled appearance along the major axis. The central bulge appears to be moderately luminous. The galaxy does not present any obvious signs of a major merger or strong tidal interactions. There may be some minor disturbances or asymmetric features within the disk structure. Overall, the galaxy exhibits a structure consistent with that of a relatively massive and mature spiral.