The galaxy exhibits a notable disk structure with a prominent blue hue, suggesting ongoing star formation. While a well-defined spiral arm structure is not immediately apparent, subtle hints of spiral arms or flocculent structures can be seen within the disk. There is no clear bulge present, but there appears to be a slight brightening toward the center of the galaxy. The light appears somewhat diffuse, suggesting a low surface brightness. There is evidence of some type of disturbance or possible merger, given the irregular morphology, and the asymmetric distribution of light within the galaxy.
