The galaxy presents as a disk-shaped structure, viewed at a near edge-on orientation. A prominent dust lane is observed bisecting the galaxy along its major axis, obscuring the central bulge. The bulge itself appears small and relatively faint. Faint spiral arm structures are visible extending outward from the bulge, primarily on either side of the dust lane. These arms appear somewhat clumpy and loosely wound, suggesting the presence of ongoing star formation. There is evidence of minor tidal disturbances, indicating that the galaxy may have experienced a recent interaction. It has a generally smooth appearance with some signs of features. There is no strong central concentration in the galaxy.
