The galaxy appears to be a spiral galaxy observed edge-on. A prominent dust lane bisects the galaxy's disk, obscuring the light from stars and gas behind it. The central bulge is bright and concentrated, appearing slightly rounded in shape. The disk itself seems relatively thin, with an estimated physical radius of approximately 2 kpc. The overall color of the galaxy is predominantly blue, suggestive of ongoing star formation within the disk. No signs of major mergers or tidal disturbances are visually apparent, though there is a slight warping to the galaxy's disk. From its morphology, it appears the galaxy is likely undergoing limited star formation.
