The galaxy presents a distinct spiral morphology. Its structure exhibits a prominent central bulge, appearing slightly elongated. Two main spiral arms are clearly discernible, winding outwards from the central bulge. These arms appear somewhat patchy, suggesting variations in stellar density and ongoing star formation regions within them. The overall color profile indicates a mix of stellar populations, with bluer regions potentially indicative of younger stars and ongoing star formation, while yellower/redder regions suggest older stellar populations. There seems to be some degree of asymmetry or distortion in the spiral structure, potentially indicative of gravitational interaction or recent minor merger.
