The galaxy presents as a disk-shaped structure, viewed nearly edge-on. There is a prominent central bulge that appears relatively smooth and rounded, exhibiting a concentrated luminosity. The disk itself appears thin, with hints of internal structure, though the resolution limits definitive identification of spiral arms or dust lanes. The disk exhibits color gradients, with a suggestion of bluer hues towards the outer edges, and redder tones closer to the bulge. The overall morphology suggests the galaxy has not experienced any recent major merger events. Slight asymmetries in the disk's light distribution might indicate minor gravitational interactions or internal dynamics.
