The galaxy presents as a face-on spiral, exhibiting a distinct disk structure. Spiral arms are clearly visible, possessing a relatively medium winding. The galaxy appears to have two dominant spiral arms. A bar structure is present across the center of the galaxy. The central bulge is moderately sized. The color profile suggests ongoing star formation, with bluer regions concentrated within the spiral arms and a slightly redder, more evolved stellar population in the bulge. There are no signs of any merging events with other galaxies.