The galaxy presents as a relatively face-on spiral galaxy with a notable disk structure. Distinct spiral arms are observed, exhibiting a somewhat flocculent morphology. Star formation appears to be actively occurring within these arms, suggested by their bluish hue. The bulge component exhibits a moderate size relative to the disk, and appears to be mostly red in color. Some morphological disturbance is evident; the spiral arms are not uniform and appear disrupted, implying possible interactions or recent mergers. The galaxy is barred, and has moderate arm winding. There may be a higher rate of star formation along the bar.
