The galaxy presents a clear spiral morphology with prominent, loosely wound arms. The central bulge appears moderate in size relative to the disk. Dust lanes are visible within the spiral arms, contributing to the patchy appearance of the disk. The overall color of the galaxy suggests ongoing star formation, particularly within the spiral arms, however it is not a particularly active one. The galaxy exhibits a possible weak bar structure. There are no signs of major tidal disturbances or ongoing mergers; however, there is the possibility of minor interaction with other objects. The galaxy is not observed edge-on. The spiral structure is dominated by two distinct arms. The galaxy has a median estimated stellar mass, and moderate levels of recent star formation.
