The galaxy exhibits a distinct edge-on disk morphology. A prominent bulge is observable, displaying a rounded shape. The disk appears relatively smooth, showing some indication of subtle internal structures. No signs of a recent or ongoing major merger are apparent; however, there is some low-level disturbance in the disk. Based on its red color and small size, the galaxy is likely at a considerable distance. The galaxy's overall structure is typical of late-type spiral galaxies viewed edge-on.
