The observed galaxy appears to be a spiral galaxy, exhibiting a flattened, disk-like structure. It is inclined at a near edge-on angle relative to our line of sight. The presence of spiral arms is suggested by subtle color variations across the disk, but the high inclination makes a definitive arm count difficult. The central bulge region is relatively prominent, appearing as a bright, concentrated region, but not extremely large relative to the rest of the galaxy. There is some suggestion of a central bar, and the spiral arms seem to have a tightly wound morphology. There is no apparent major merging or significant tidal disturbance.
