The galaxy presents as a face-on spiral with a prominent, tightly wound spiral structure. Multiple arms are discernible, although a precise count is somewhat obscured by their complex morphology. The arms appear patchy, exhibiting variations in luminosity and color, suggesting active star formation regions interspersed with areas of lower stellar density. The central bulge is relatively small and diffuse compared to the disk, exhibiting a yellowish hue indicative of an older stellar population. There is no obvious bar structure. The overall impression is of a well-defined spiral with some degree of internal disturbance, possibly indicating minor gravitational interaction, but no major merging event.
