The observed galaxy presents as a spiral galaxy with a distinct disk structure, although the disk is not perfectly face-on. There is a central bulge, moderate in apparent size, exhibiting a bright, concentrated luminosity. Spiral arm structures are visible, appearing tightly wound around the central bulge, with a possibility of two or more arms. There appears to be a strong bar that extends through the middle of the bulge. In the disk there are some dust lanes visible. There are no obvious signs of major mergers; however, there is a possible minor disturbance within the structure.
