This galaxy presents a distinct spiral morphology. Two prominent spiral arms are visible, loosely wound and extending outwards from the central bulge. The bulge appears relatively small and subdued compared to the overall galactic disk. The disk exhibits a mottled texture indicative of active star formation regions within the spiral arms, appearing as areas of enhanced luminosity and bluer color. There is also a hint of a bar-like structure in the very central region of the galaxy. There is a clear color gradient visible, with bluer hues observed along the spiral arms and a redder hue in the central bulge. The spiral structure dominates the galaxy's form, with the arms being more prominent than the bulge. There is no evidence of a major merger, but the irregularities in the spiral arms may suggest minor gravitational interactions. The galaxy is not observed edge-on, so its spiral form is clearly defined from this viewing angle.