The galaxy appears to be a spiral galaxy, observed at an oblique angle relative to its disk. The disk component exhibits distinct spiral arm structure, although the arms appear somewhat flocculent and asymmetrical. A central bulge is present, displaying a yellowish hue indicative of an older stellar population. The disk itself shows a bluer color, suggesting ongoing star formation. There may be a bar structure within the central regions. The galaxy shows possible signs of minor disturbance and an elongated morphology, suggesting potential gravitational interaction with another galaxy. The outer regions of the galaxy have low surface brightness, making it difficult to discern the full extent of the disk.
