The galaxy exhibits a complex morphology, appearing as a system potentially undergoing a merger or interaction. One component presents a smoother, less structured appearance, with a more diffuse light profile that is more yellowish in color. The other component appears more disturbed, with a significant color gradient. This component shows a distinct red core with a brighter central region, surrounded by a bluer, less-defined halo. This may indicate an actively star-forming region or a population of younger, hotter stars within this halo. There may be minor disturbances present in the form of tidal tails or distorted features, though the resolution limits definitive confirmation. The galaxy exhibits an intermediate roundness, deviating from a perfectly circular shape. The overall color suggests an intermediate redshift galaxy.
