This galaxy exhibits a flattened, disk-like morphology, suggesting it is a spiral or lenticular type galaxy. The disk is viewed at a moderate inclination angle. There is no distinct central bulge, however a smooth region is visible in the central region of the galaxy. Patches of bluer light are present in the galactic disk, potentially indicating regions of recent star formation. Some asymmetries in the disk's structure are present with a possible disturbance in its morphology. An elongated, amorphous structure is suggested in the center of the galaxy. There is no evident active galactic nucleus. Overall, the galaxy appears to be a relatively low-mass system with a low star-formation rate.
