The galaxy presents as a somewhat face-on spiral structure, although the arms are not sharply defined. The central bulge appears prominent and exhibits a yellow-orange hue, indicative of an older stellar population. The spiral arms are bluer in color, suggesting ongoing star formation. The disk structure seems relatively smooth with a few minor disturbances apparent. The galaxy has an elliptical shape, it is more rounded than cigar shaped. There is no major or ongoing merging. 
