This galaxy presents as an edge-on spiral, exhibiting a clear disk structure with a prominent central bulge. Dust lanes are apparent, obscuring some of the disk's light and creating a mottled appearance along the galactic plane. The bulge region displays a smoother, more concentrated light distribution suggesting an older stellar population. There appears to be some star formation present, signified by the presence of bluer regions within the disk, although these regions are not as sharply defined. Overall, the galaxy appears relatively undisturbed, with no obvious signs of a recent major merger.
