The galaxy presents as a spiral type, exhibiting well-defined spiral arms. The winding of these arms appears to be generally medium in tightness. It's possible that there are two main spiral arms, although that determination could be improved with better resolution. The central bulge is moderately sized relative to the disk and has a yellowish hue. The disk of the galaxy shows blue regions, indicative of younger, hotter stars within star-forming regions. There appears to be a slight asymmetry or disturbance in the morphology of the galaxy, possibly indicating minor gravitational interaction. The overall color suggests ongoing star formation.
