The galaxy appears as an edge-on spiral with a clearly defined disk. The dust lane is visible, bisecting the galaxy's light along its major axis. There is evidence of a central bulge, which appears rounded in shape. The disk appears relatively smooth with no prominent spiral arm structures discernible. The galaxy is relatively isolated and shows no obvious signs of tidal disturbances or interactions with neighboring galaxies. Overall, it has a regular morphology indicative of a stable, undisturbed system.
