The galaxy presents a prominent, well-defined spiral structure. The arms exhibit a grand design, tracing a clear and organized pattern around the galactic center. The winding of the spiral arms appears moderate, not tightly wound nor overly loose. Two dominant spiral arms are clearly visible. There appears to be a strong central bar structure bisecting the galaxy’s core. The bulge is small relative to the disk size. The disk appears relatively flat. There is evidence of ongoing or recent interactions influencing its morphology, indicated by disturbances to the spiral arm structure. The galaxy is not undergoing a full merger, but exhibits noticeable irregularities. The presence of star-forming regions is implied by the variations in color and brightness within the spiral arms.
