The galaxy appears to be a spiral type, exhibiting a flattened disk structure. A prominent central bulge is observable, though it does not appear to be the dominant feature. The spiral arms are readily apparent, exhibiting a tightly wound structure. The winding is well-defined. The arms themselves appear somewhat flocculent in nature, showing areas of clumpy star formation regions. Patches of blue light can be seen, indicating ongoing star formation activity within these regions. Overall the galaxy seems to be relatively undisturbed with no major signs of merging activity. There appears to be no significant bar structure within the galaxy.
