This galaxy appears to be a spiral galaxy observed nearly edge-on. There is a bright, concentrated central bulge, which appears yellowish, suggesting an older stellar population. A faint, elongated disk extends from the bulge. The disk is oriented vertically in the image and seems to have a relatively high degree of symmetry. There is a hint of dust lane obscuration along the galactic plane, although it is not distinct, suggesting it may be a galaxy with little star formation. The galaxy does not appear significantly disturbed.