The galaxy presents a clear spiral structure. Two prominent arms emanate from a central bulge, tracing a path around the galactic core. These spiral arms appear well-defined and somewhat tightly wound, with noticeable regions of star formation exhibiting a bluer hue interspersed within the arms' overall structure. The bulge itself has a yellow-orange color, which may indicate an older stellar population within that central region.

Overall, there is a lack of evidence to suggest this galaxy is undergoing a major merging event. There may be a slight disturbance in one of the arms but nothing to suggest any major mergers. The image data indicates it's a spiral galaxy dominated by its disk features. The nucleus shows a lack of a strong bar structure. The presence of spiral arms is readily apparent.

