The galaxy exhibits a distinct spiral structure, with a prominent central bulge that fades gradually into a disk. The spiral arms are moderately defined, displaying a somewhat flocculent morphology. There appears to be some degree of asymmetry or irregularity in the arm structure, possibly indicating gravitational interaction or disturbance. The colour gradient suggests the presence of active star formation within the disk, particularly along the spiral arms. The light is fairly blue, indicating younger, hotter stars. A central bar might be subtly present but is not clearly defined. There are possible signs of tidal features or a minor merger event. There is a lower concentration of light in the galactic center, possibly due to the presence of dust.
