The galaxy presents as an edge-on spiral, exhibiting a clearly defined disk structure. The galactic bulge appears prominent and concentrated, exhibiting a smooth, rounded morphology. There is a visible dust lane bisecting the galaxy, obscuring a portion of the bulge light. The overall color profile suggests a mix of stellar populations, with bluer colors concentrated in the disk and redder colors dominant in the bulge. The disk appears somewhat disturbed or warped, and a possible tidal tail is visible emanating from one end of the galaxy. There is also a small region of star formation. This region is distinct in color and appears to be very active. This could be the result of a minor merger.
