The galaxy appears to be a spiral galaxy, seen almost perfectly edge-on. A prominent central bulge is visible, with a rounded morphology. The disk component is thin and elongated. There is some suggestion of dust lane obscuration along the galactic plane. A small amount of irregularity may be visible within the disk. The overall color of the bulge is redder than the disk. The galaxy appears relatively isolated, with no obvious signs of major tidal interaction or ongoing merger activity with any companion galaxy.
