The galaxy presents as an elongated, disk-like structure viewed edge-on. A central bulge is subtly visible, although its prominence is relatively subdued. The disk exhibits a smooth texture with no distinct spiral arm features or prominent dust lanes directly observable, though a slight colour variation across the disk suggests some internal structure. The galaxy's overall colour appears bluish-white, suggesting the presence of relatively young stars and ongoing star formation processes, albeit at a low rate. There is no immediate visual evidence of a major ongoing merger, but some minor disturbances cannot be ruled out.
