The galaxy presents as a spiral type, characterized by a central bulge and a prominent disk. The central bulge appears relatively compact with a yellow hue. The disk component is not viewed perfectly face-on, but at a slight inclination. Spiral arms emanate from the central region and extend outwards. A distinct winding of the spiral arms can be observed, and there appear to be two clearly defined spiral arms. The arms are somewhat patchy in appearance, displaying both areas of brighter emission, possibly indicating regions of active star formation, and areas of lower surface brightness. The blue color of the arms may be a result of the presence of young, hot stars. There is some indication of a bar-like structure extending from the center. There is no visual evidence of a major merger. The morphology of this galaxy suggests it is an actively star-forming spiral galaxy.
