The galaxy presents a flattened disk-like morphology, viewed at an angle that is somewhat face-on. A prominent central bulge dominates the inner region, appearing relatively smooth and concentrated. The color of the bulge appears to be more yellow-orange, suggestive of an older stellar population. Fainter spiral arm structures seem to emanate from the bulge. The arms are not sharply defined. The outer disk appears more diffuse with bluer patches, possibly indicating ongoing star formation regions scattered throughout. Overall, the galaxy appears to be an intermediate spiral type, not tightly wound, nor highly irregular. It has a relatively high degree of symmetry in the distribution of light and color. There does not seem to be any evidence of a major merger, but there could possibly be a minor disturbance present.
