The galaxy presents as a spiral with a well-defined structure. The spiral arms are prominent and tightly wound close to the center. The arms extend outwards, becoming less distinct. The central bulge appears small relative to the disk. A strong bar structure traverses the galaxy's center. The color distribution suggests active star formation within the spiral arms, seen through the varying luminosity. There appear to be some minor disturbances in the galaxy shape, and there appears to be merging happening.
