The galaxy presents a complex morphology, appearing as a spiral galaxy with a significant level of ongoing interaction or disturbance. The spiral arms are prominent and exhibit a multi-armed structure with a mix of tightly and loosely wound segments. A bar structure is present, though not exceptionally strong, extending through the galactic center. The central bulge appears to be of moderate size compared to the overall disk. Patches of intense star formation are evident throughout the arms, visible as bright knots and regions of bluer light. The overall color suggests active star formation, with a notable blue component interspersed with regions of older, redder stellar populations. There are some signs of possible tidal features or disturbances, suggesting the galaxy may be undergoing or have recently experienced a minor merger or gravitational interaction. The disk of the galaxy is tilted relative to our line of sight, presenting a face-on to intermediate inclination.
