The galaxy presents a disk-like structure, viewed at an oblique angle relative to our line of sight. The central region exhibits a concentrated luminosity, suggesting a prominent bulge component. The color of the bulge appears yellowish, indicative of an older stellar population. Fainter, diffuse spiral arms extend from the central bulge, displaying a bluer hue, implying ongoing star formation. There are morphological disturbances within the disk and throughout the galaxy. These disturbances seem significant, and could be due to a major merging event. The disk's morphology indicates the absence of a strong bar structure. Overall, this galaxy is likely in the midst of a major disturbance or merger.
