This galaxy presents a clear spiral structure. The arms are well-defined and loosely wound, extending outwards from a central region. Two prominent spiral arms are easily discernible. A faint bar-like structure appears to bisect the galaxy's core, with an orientation along the East-West axis. The central bulge is not dominant, appearing small to moderate in size. There are some signs of disturbance in the galaxy's morphology, possibly suggesting a minor interaction or past merger event. The colour distribution indicates active star formation occurring within the spiral arms, as evidenced by bluer regions. The overall colour of the galaxy is consistent with a system containing both young, hot stars and older stellar populations. The disk of the galaxy appears face-on. 
