The galaxy presents as an edge-on spiral, exhibiting a prominent, elongated disk with a central bulge. The bulge appears somewhat rounded, with the disk showing only minor internal structure. There is evidence of dust lanes, causing some obscuration along the plane of the disk. The disk also shows indications of recent or ongoing star formation, supported by a hint of bluer regions. Overall, the system appears relatively undisturbed, lacking any significant signs of tidal interactions or major mergers.
