The galaxy presents a distinct spiral structure, evident despite the image's resolution. The spiral arms appear tightly wound around a prominent central bulge. The bulge exhibits a yellowish hue, suggesting a concentration of older stellar populations. The spiral arms display a bluer tint, indicative of ongoing star formation activity. The galaxy's disk shows a relatively high degree of inclination with the galactic plane, but the disk can still be observed as it extends along the major axis with the arms. There are no readily apparent signs of major mergers or significant tidal disturbances, and the galaxy appears relatively isolated. Evidence suggests a moderate rate of star formation within the arms. 
