The galaxy presents a spiral morphology. Its arms are somewhat loosely wound and exhibit a flocculent structure. The central bulge appears prominent and displays a yellowish hue, possibly indicative of an older stellar population. The spiral arms show hints of bluer regions, suggesting ongoing star formation within them. The galaxy appears to be undergoing a merger event, based on the disturbed morphology and visible tidal tails. There is an indication of possible minor interaction with another object nearby.
