This galaxy exhibits a spiral morphology with a prominent central bulge. The spiral arms are tightly wound and display a flocculent structure. Two main arms are clearly visible extending outwards from the bulge region. The bulge appears yellowish indicating older stellar populations, while bluer hues in the arms suggest ongoing star formation. The galaxy's disk is viewed at a moderate inclination. No signs of a strong central bar are visible. The overall shape does not suggest any ongoing major merger activity, though a slight distortion or minor tidal feature cannot be ruled out.
