The galaxy presents as a relatively face-on spiral with a discernible central bulge. The spiral arms exhibit a somewhat flocculent structure, appearing patchy rather than continuous. There appears to be ongoing star formation activity within the arms, as evidenced by localized regions of bluer coloration, suggesting the presence of younger, hotter stars. The overall color of the galaxy is slightly blue, but towards the center it appears to be more yellow. There is no obvious bar structure. 
