The galaxy presents as a moderately inclined spiral with evident features. It appears somewhat flocculent in structure, exhibiting fragmented spiral arm segments rather than well-defined, continuous arms. There are sections where the blue hue indicates areas of active star formation along the arms. 

The central bulge of the galaxy is either small or non-existent and the lack of a large central condensation suggests a relatively low stellar density in that region. The galaxy may have a faint bar feature that is only slightly discernible. The galaxy does not appear to be undergoing a major merger, though it could be experiencing minor gravitational interactions, as its morphology suggests a disturbed or asymmetric shape.
