The observed galaxy presents as a spiral type. Evident spiral arms emanate from a prominent central bulge, and the disk is viewed at an angle slightly offset from face-on. The spiral arms appear somewhat tightly wound near the core, transitioning to a more open structure as they extend outward. The overall color of the galaxy suggests ongoing star formation, particularly within the spiral arms, with bluer hues dominating these regions. The central bulge exhibits a yellower color, potentially indicating an older stellar population. Morphological irregularities suggest possible gravitational interactions or a recent merger event, evidenced by asymmetry in the disk and disrupted arm structure. Some sections of the arm structure appear disturbed. This galaxy showcases characteristics of both established structure and ongoing dynamic processes.
