The galaxy presents a discernible disk structure, though its features are not sharply defined. The central bulge appears prominent and exhibits a yellowish hue, suggesting a population of older stars. From the disk emerge spiral arms. They appear grand and well-formed, tightly wound around the galactic center. The color of the spiral arms indicates active star formation. Based on its appearance, this is a relatively massive galaxy with an active star formation rate. There is no evidence of any major mergers and it is not an edge-on galaxy. A small bulge suggests a spiral winding.
