This galaxy presents as an edge-on spiral, with a prominent dust lane bisecting the galactic plane. The central bulge appears elongated. Moderate star formation is indicated by the presence of bluer regions along the outer edges of the disk, contrasting with the more yellow/orange hues of the central bulge, which could indicate an older stellar population. The disk appears relatively smooth, with minimal signs of major disturbances or ongoing mergers, though slight asymmetries in the outer disk regions cannot be ruled out due to the viewing angle. The bulge appears to be somewhat rounded.
