The galaxy presents as a flattened, disk-shaped structure oriented edge-on with respect to our line of sight. The central bulge is subtly brighter than the surrounding disk, exhibiting a smooth, concentrated light distribution, indicating an older stellar population residing there. The disk itself appears relatively smooth, though some subtle variations in luminosity may suggest underlying spiral arm structures that are difficult to discern due to the edge-on viewing angle.

The overall color is slightly bluish, particularly towards the outer edges of the disk. This bluer hue suggests the presence of younger, hotter stars and ongoing star formation within the disk. The distribution of this blue light is not entirely uniform, possibly indicating localized regions of more intense star formation. There are no obvious signs of major tidal disturbances or ongoing mergers. The galaxy presents an undisturbed form.
