The galaxy presents as a flattened, disk-shaped system, observed nearly edge-on. A central bulge is prominent, displaying a yellowish-orange hue, suggestive of an older stellar population. The disk itself exhibits a bluish tint, likely indicating ongoing star formation. The light is somewhat disrupted. One section of the disk appears slightly warped. There is no apparent active galactic nuclei. The galaxy shows signs of minor tidal disturbances or ongoing interactions, as evidenced by the subtle asymmetries in the outer disk.
