The galaxy exhibits a spiral morphology, characterized by prominent spiral arms emanating from a central bulge. The arms appear tightly wound in the inner region, transitioning to a more open structure as they extend outwards. Patches of blue light are visible within the spiral arms, indicating regions of active star formation, likely associated with the presence of hot, young stars. The central bulge presents a smooth, concentrated light distribution, suggesting an older stellar population. A bar-like structure appears to run through the center of the bulge, indicating that this may be a barred spiral galaxy. The disk is viewed at an angle. Overall, the galaxy displays characteristics of an evolved spiral galaxy with ongoing star formation.
