The galaxy presents a complex morphology, exhibiting characteristics of a spiral galaxy undergoing a significant interaction or merger. A central, bright bulge region is visible, indicating a concentration of older stellar populations. Emanating from this bulge are discernible spiral arm structures. These arms appear somewhat irregular and disrupted, hinting at gravitational disturbances. One arm appears tighter in winding than the other, with the arm that is more loosely wound exhibiting a bluer color, indicative of active star formation. The overall color profile of the galaxy suggests a mix of stellar populations, with younger, bluer stars present in the spiral arms and older, redder stars concentrated in the bulge. An asymmetric distribution of light and color throughout the galaxy further supports the likelihood of an ongoing interaction or recent merger event that could have perturbed the galaxy's original structure. Patches of concentrated color are dispersed throughout the galaxy, indicating regions of active star formation.
