The galaxy presents a spiral morphology, observed at a slight inclination. It exhibits a prominent central bulge, surrounded by a disk component displaying clear spiral arm structure. The spiral arms appear relatively loosely wound and traced by regions of active star formation, indicated by blue-shifted light. A bar structure transects the galactic center, oriented at an angle to the major axis of the disk. The overall color of the galaxy suggests a mix of stellar populations, with younger, bluer stars concentrated in the arms and older, redder stars dominating the bulge. The disk shows a moderate amount of dust obscuration, particularly along the spiral arms. There may be a hint of some tidal disturbance.
