The galaxy exhibits a prominent disk structure, viewed at an angle intermediate between face-on and edge-on. Spiral arms are evident, although somewhat indistinct due to the viewing angle and likely moderate redshift. These arms appear tightly wound around the central bulge. The central bulge itself is of moderate size and appears relatively bright. The overall color suggests moderate levels of ongoing star formation. There is no obvious presence of a bar. The outer regions of the disk show some disturbance in the morphology, possibly due to minor interactions with smaller galaxies or past merger events, but it is also possible these are just the irregular structures of the spiral arms. The galaxy does not display a merging event in progress.