The galaxy presents a generally smooth morphology with a hint of features suggesting a disk. The light distribution indicates a nearly round shape, with a slight departure from perfect circularity. The galaxy exhibits an orange hue, suggesting a population of older stars and/or significant dust obscuration. Evidence of a potential interaction is noted, possibly in the form of tidal tails or distortions in the main galactic body. The main galaxy is potentially in the late stages of merging with another galactic object. The system exhibits a degree of disruption, which might be the result of such ongoing interaction.
