The galaxy exhibits a spiral structure, with prominent arms extending from a central bulge. The arms appear somewhat tightly wound. The bulge is moderately sized and displays a yellowish-white hue, possibly indicating an older stellar population. There may be a bar structure present across the central region of the galaxy.

The spiral arms show color variations, with bluer regions interspersed amongst a more general distribution of color. The spiral arms could have recent star formation present, but the color is muted. There are no signs of a major merger; the spiral arms look relatively undisturbed. 
