The galaxy exhibits a disk morphology, though the viewing angle is such that it is significantly inclined relative to our line of sight, but not entirely edge-on. Two spiral arms seem to be present although it is difficult to discern exact count and overall appearance. The spiral arms themselves appear tightly wound. The central bulge of the galaxy is not dominant, and is relatively small. The color of the galaxy indicates a mix of stellar populations, likely including both older, redder stars in the bulge and younger, bluer stars in the spiral arms. There is a small presence of dust lanes within the spiral arms. No strong bar structure is apparent within the galaxy. The galaxy exhibits no significant signs of major mergers or strong tidal disturbances. It is difficult to tell whether the galaxy has a minor disturbance.
