The galaxy presents as a relatively well-defined spiral structure. The central bulge appears moderately sized and exhibits a yellow-orange hue, potentially indicating an older stellar population. Emanating from the central bulge are multiple spiral arms which seem tightly wound close to the center and loose as they reach the edge. The spiral arms contain regions of blue-white light, suggesting areas of active star formation. The arm structure is somewhat uneven, with areas showing signs of disturbances or distortions, possibly indicative of minor gravitational interactions or internal dynamic processes. There is no strong evidence of a bar-like structure. No clear signs of an ongoing major merger are visible; however, subtle asymmetries might suggest minor interactions or tidal disturbances. The galaxy's disk is viewed face-on. Overall the galaxy seems to be undergoing considerable star formation.