The galaxy presents as a somewhat diffuse, face-on spiral with a centrally concentrated bulge. The color appears generally bluish, suggesting the presence of younger, hotter stars. The spiral arms are not very well defined, but the overall structure shows some irregularities and clumpy star formation regions throughout. There is minimal evidence of a strong, distinct disk; it appears more like a diffuse, feature-rich system. There's also the possibility of minor tidal disturbances or interaction with another nearby galaxy. Overall, it seems to be a galaxy with ongoing star formation and moderate levels of star formation activity. The galaxy's roundness is between an ellipse and a circle.
