The galaxy presents a clearly defined disk structure oriented approximately edge-on relative to our line of sight. The central bulge region appears moderately prominent, exhibiting a somewhat condensed morphology. Faint spiral arm structures can be discerned extending outwards from the bulge, though their definition is somewhat diffuse. There is an indication of dust lane features visible across the disk, obscuring some of the light from the galactic plane. The galaxy is roughly elliptical in shape. The overall color appears to be bluish, especially at the outer edges, suggesting a younger stellar population within the disk. There is no evidence of a major ongoing merger or significant tidal disturbances.
