The galaxy presents a morphology consistent with a spiral type. A central bulge region is visible, appearing moderately bright with a yellowish hue suggesting an older stellar population. Extending outwards are defined spiral arms exhibiting a medium winding. The spiral arms show a clumpy, knotty structure, which suggests active star formation regions. The color of the arms is predominantly bluish, indicative of younger, hotter stars. The galaxy's overall shape is somewhat disturbed or asymmetric, indicating a possible interaction with another galaxy, or a recent merger event. A bar structure may or may not be present. It is difficult to tell from the image. The galaxy is not edge-on. There are most likely two to three clearly identifiable spiral arms. The morphology suggests a galaxy undergoing some type of gravitational disturbance.
