The galaxy presents as an edge-on spiral, exhibiting a prominent dust lane bisecting its disk. The central bulge appears bright and concentrated, with a somewhat rounded morphology. The disk itself is relatively thin and elongated, with a visible difference in color between the central region and the outer edges. The core presents a warmer tone, suggesting an older stellar population. The dust lane is well-defined and appears relatively undisturbed, indicating that the galaxy may not have experienced a recent major merger. There are some signs of subtle disturbances in the morphology of the disk, such as a slight warping, and a lower amount of recent star formation. Overall, the galaxy appears to be an evolved spiral galaxy observed at a considerable distance, with a well-defined structure and signs of relatively quiescent activity.
