The galaxy presents a complex morphology suggestive of an intermediate spiral type. A prominent, moderately sized bulge is visible, exhibiting a somewhat diffuse appearance. Spiral arms appear loosely wound and somewhat flocculent. The disk shows varying degrees of brightness, with hints of dust lanes partially obscuring the galactic center. The galaxy appears to show signs of potential interaction or merging activity, given some irregular features in its structure. A stellar bar appears to be present across the galactic center. Star formation seems to be present. The galaxy appears to be rotating.