The galaxy presents as a face-on spiral with well-defined spiral arms, a bright central bulge, and a disk component. The central bulge appears yellow/orange, suggesting an older stellar population. The spiral arms are visible, although somewhat flocculent and not as sharply defined as grand design spirals. There is a clear blue tint to the arms, indicating ongoing star formation. The arms extend fairly far out from the center. There is no strong evidence of a bar structure. There do not appear to be any major signs of a recent or ongoing major merger. Faint areas of diffuse light surround the disk.
