The galaxy presents as a spiral type with a prominent central bulge. The spiral arms are clearly visible, extending outwards from the bulge. The morphology indicates a relatively high likelihood of spiral arms present, and a low likelihood of the galaxy being edge-on. The arms exhibit a winding pattern, appearing moderately tight. The spiral arm count is difficult to ascertain definitively from the image, but likely consists of two to three arms. The overall structure does not show significant signs of major disturbance or merging activity, appearing relatively settled. The galaxy exhibits a range of colors, suggesting a mix of stellar populations. The redder colors likely indicate older stars in the bulge. bluer colors may represent younger stars within the spiral arms.
