The galaxy presents a distinct spiral structure with well-defined arms extending from a central bulge. The spiral arms appear loosely wound, with a flocculent morphology. The central bulge exhibits a moderate size relative to the disk. Patches of star formation regions are noticeable within the spiral arms, marked by a bluer color, indicating the presence of young, hot stars. The overall color of the galaxy suggests a mix of stellar populations, with a yellow-red hue dominating in the bulge. The galaxy's disk appears to be viewed at a relatively face-on inclination.
