The galaxy presents as a spiral type, with a notable disk structure. The spiral arms are loosely wound, extending outwards from a central bulge region. The arms are not perfectly symmetrical, displaying a slightly flocculent morphology. The color distribution suggests active star formation within the spiral arms, particularly in the outer regions, which exhibit a bluer hue. A moderate bulge is visible, though it doesn't appear to dominate the overall structure. There's a suggestion of a bar feature across the central region, though not strongly defined. There may be some minor disturbances or interactions occurring, but the primary structure is not significantly disrupted. The galaxy is not seen perfectly edge on, providing a clear view of the spiral pattern.
