The galaxy appears to be a spiral galaxy, with a notable disk structure. Arm structures appear fragmented and somewhat clumpy with some regions of enhanced intensity and color variation, suggestive of ongoing star formation. The color in these regions appears more blue, which supports ongoing star formation. The disk is not perfectly flat and has some slight irregular features, suggestive of tidal disturbance or interaction. There appears to be a bulge. Evidence of past or ongoing merger activity is present. It is an object undergoing some sort of merging process. There is no strong obvious bar feature. The dust content is unknown given the resolution, though color variations are present.