The galaxy presents as a late-type spiral galaxy, oriented nearly edge-on with respect to our line of sight. A prominent dust lane is visible bisecting the galaxy, obscuring the central bulge. The bulge itself appears elongated and somewhat diffuse, with a color gradient suggesting an older stellar population. Faint, diffuse spiral arms extend outward from the central region and show hints of blue light. The galaxy does not exhibit any signs of major mergers or strong tidal disturbances and shows a smooth disk.
