The galaxy presents as an edge-on spiral, exhibiting a flattened disk structure. A pronounced central bulge is evident, appearing relatively smooth. Dust lanes are visible along the plane of the disk, obscuring some of the light from the bulge. The disk displays a blueish hue at the outermost edges, potentially indicating regions of active star formation. The majority of the disk light is emitted at redder wavelengths. Overall, the galaxy is characterized by a strong disk component and a less prominent bulge. No obvious signs of a major merger or tidal disturbances are apparent in the image.