The galaxy presents a complex morphology, appearing as a merging system comprised of at least two distinct components. One component exhibits a smoother, more rounded structure with a yellowish-orange hue, indicative of an older stellar population. This component appears relatively undisturbed, lacking prominent spiral arms or other features of active star formation. The other component displays a bluer color, suggesting the presence of younger, hotter stars and potentially ongoing star formation. This component appears slightly more amorphous and irregular in shape, and could indicate a disk-like structure. The system exhibits a faint tidal bridge of material connecting the two components, suggestive of an ongoing interaction. While the system is not dramatically disrupted, there appears to be some distortion in the overall structure of both galaxies. The relative sizes of the components are similar.
