This galaxy presents an edge-on morphology, displaying a flattened disk structure. A central bulge region is clearly visible, appearing rounded and slightly elongated. Dust lanes are readily apparent, obscuring portions of the disk, particularly closer to the midplane. These dust lanes exhibit a reddish hue, suggestive of the presence of interstellar dust absorbing blue light.

The disk itself displays a gradient in color, becoming bluer towards the outer edges, which indicates areas of more active star formation in the outer regions of the disk. A faint halo may be present, with a roughly estimated mass of 10^10 solar masses, this might suggest a spiral galaxy. We can observe the red shift in the image.
