The galaxy presents a clear disk structure, with a discernible central bulge. The disk exhibits a dominant spiral arm morphology. The arms appear tightly wound, and the number of arms present is difficult to ascertain from this image. The galaxy appears to be largely unperturbed, showing no indications of major merging activity. A bar structure is not prominently visible. The bulge size seems moderate in size when considering the disk size. The overall color index suggests a mix of stellar populations, with bluer regions likely associated with ongoing star formation within the spiral arms and a yellower central bulge indicative of an older stellar population.
