The galaxy exhibits a complex morphology, suggestive of an ongoing or recent interaction or merger event. Two distinct nuclei are visible, each with a concentrated central region of older stars exhibiting a yellowish hue. A diffuse, asymmetric structure surrounds the nuclei, exhibiting a bluish tint likely indicating regions of active star formation. Extended tidal features are not readily apparent within the image, but the overall disturbed morphology points to a history of gravitational interaction. The galaxy displays characteristics indicative of a spiral galaxy, though the interaction has visibly distorted the original spiral structure. Star formation appears to be active, primarily distributed throughout the galactic disk. There is no discernible bar structure within the galaxy. The bulge size is small relative to the overall galaxy size. The galaxy shows a slight disk-like shape and may be interacting or merging with another galaxy. The winding of any potential spiral arms cannot be confidently determined.
