The galaxy presents as a spiral structure, oriented approximately face-on relative to our line of sight. The spiral arms are tightly wound, exhibiting a high degree of coiling around the central bulge. These arms are not uniform; they display a clumpy morphology, suggesting regions of active star formation characterized by a bluer hue. A prominent central bulge is observed, appearing bright and concentrated. A bar feature is apparent; it spans a noticeable extent through the galaxy's core region. Overall, the galaxy exhibits a classic spiral morphology with active star forming regions and a defined bulge. No major mergers appear to be occurring. 
