The galaxy exhibits a distinct spiral structure, with prominent, loosely wound arms extending from the galactic center. Two spiral arms are clearly discernible. The arms display clumpy regions of star formation, indicated by their slightly brighter and uneven appearance. The central bulge appears relatively small. There appears to be a weak bar structure that crosses the center of the galaxy. There may be ongoing, minor gravitational disturbances or interactions impacting the system. Overall, the galaxy displays a classic spiral morphology with indications of recent or ongoing star formation activity.