The galaxy presents as a spiral type, with a notable disk structure. The spiral arms appear tightly wound. A bar feature is clearly visible bisecting the central region of the galaxy. The bulge appears relatively small in proportion to the overall disk size. There is no obvious sign of recent or ongoing major merger activity, though some minor irregularities in the disk's morphology might suggest tidal interactions or minor disturbances. The overall color of the galaxy suggests active star formation, especially in the spiral arms.