The galaxy presents as a relatively faint, elongated object. Its morphology appears to be disc-like and is observed edge-on. A central bulge is subtly discernible, exhibiting a slightly brighter and more diffuse region compared to the surrounding disc. The disc shows some evidence of internal structure, though the resolution limits detailed analysis. There's a suggestion of dust lanes or obscuration along the equatorial plane, manifesting as subtle dark variations. The galaxy's overall color is somewhat red, suggestive of an older stellar population and potentially lower star formation activity. No prominent spiral arms are visible, consistent with its edge-on orientation. The apparent smoothness of the disc could indicate a lack of significant recent mergers or major disturbances. However, a very slight warping or asymmetry cannot be completely ruled out given the available resolution.
