The galaxy appears to be a spiral type, seen at a relatively face-on angle. It exhibits a prominent central bulge, with a yellowish hue, suggesting an older stellar population. Two main spiral arms are visible, emanating from the central region. These arms appear somewhat tightly wound closer to the bulge, and show medium winding towards the edges, giving a more flocculent appearance.

The arms appear to be populated with both older stars and regions of active star formation, indicated by a bluer color in some sections, although this is faint.

The disk is the main feature observed. There's a weak, barely perceptible presence of a bar structure crossing the central region. 
