This galaxy presents as an edge-on spiral, characterized by a flattened disk and a prominent central bulge. There appears to be a significant dust lane bisecting the galaxy along its major axis, obscuring the light from the stars and gas behind it. The bulge exhibits a slight boxy morphology, although a more rounded shape is also apparent. There is evidence of ongoing star formation, as indicated by the redder, patchy regions within the disk. Overall the galaxy shows no obvious signs of major disturbance or interaction with other galaxies.