This galaxy presents as a late-type spiral, observed nearly edge-on. A prominent dust lane bisects the galaxy along its major axis, obscuring the central bulge. The bulge appears primarily smooth and rounded. The disk appears thin and relatively undisturbed. The color of the disk is reddish, which may indicate a relatively older stellar population or significant dust obscuration. There may be some very slight distortion of the disk, which could suggest a minor merger. The overall morphology indicates a system that is dominated by the disk, although there may be some activity within the disk.