The galaxy presents as a spiral type, observed at a slight inclination. Prominent, tightly wound spiral arms are discernible, exhibiting a blue hue, suggesting active star formation within these regions. The central bulge appears relatively small and features a yellow-white coloration, indicating an older stellar population. Overall the galaxy shows a moderate amount of star formation activity, it is well defined, and appears relatively undisturbed, with no obvious signs of recent major mergers. The disk component is dominant.
