This galaxy exhibits a clear spiral structure. Two dominant spiral arms are visible, winding moderately around a central bulge. The bulge appears relatively small to moderate in size compared to the overall extent of the disk. The winding of the spiral arms appears to be intermediate, neither tightly wound nor loosely defined. The galaxy does not appear to be strongly barred. The color suggests active star formation is occurring, especially within the spiral arms, indicated by the bluer hues. There is no obvious sign of recent major mergers, however, some minor disturbance or interaction might be possible.
