This galaxy presents a distinct spiral morphology. Prominent spiral arms are visible, displaying a loosely wound structure. The galaxy's bulge appears moderate in size, contributing significantly to the overall light distribution. Evidence suggests the presence of a bar-like structure in the central region, though it may be somewhat weak. The system displays an overall blue hue, indicating ongoing star formation. There are no signs of major interactions or mergers, although there appears to be a minor disturbance with an asymmetric shape to its disk. 
