The galaxy appears to be a relatively smooth, disk-shaped system viewed nearly edge-on. The light distribution indicates a central bulge with a gradual decrease in brightness towards the outer edges. The shape of the galaxy is elongated, with a pronounced cigar-like appearance due to the viewing angle. There's a suggestion of dust lanes or other internal features obscuring the light, contributing to the overall fuzziness and lack of sharp definition. Color gradients are visible, transitioning from bluer hues at the apparent edges of the disk to redder tones towards the central bulge, suggestive of varying stellar populations and possible ongoing star formation in the disk. There may be a small indication of a minor disturbance to the galaxy's morphology.
