The galaxy displays a discernible spiral structure. Prominent spiral arms originate near the central bulge, appearing somewhat tightly wound. A weak bar-like feature appears to bisect the central bulge. The central bulge region exhibits a brighter, more concentrated luminosity, suggesting an older stellar population. The spiral arms show varying degrees of star formation, indicated by bluer patches interspersed within the arms. The disk is not viewed edge-on. There may be evidence of a minor disturbance or interaction with another galaxy. The galaxy contains two distinct arms.