The observed galaxy presents as an edge-on spiral, with a prominent dust lane bisecting the galactic plane. The central bulge appears bright and subtly boxy, with light from the bulge showing a smooth, rounded shape. The disk of the galaxy appears elongated, with a reddish hue possibly indicative of older stellar populations and dust obscuration. There are hints of disturbed morphology within the disk. There are also signs of recent or current minor interactions. Overall, the morphology suggests a disk galaxy undergoing some form of interaction.
