The galaxy presents as a luminous, yellowish-white object with an apparent smooth morphology. It appears to exhibit a somewhat spheroidal shape, although the structure is not perfectly round, showing hints of asymmetry. There is evidence of a possible interaction or merger event, given the clumpy and disturbed nature of the galaxy's light distribution. There are at least two more concentrated light-emitting areas, indicating the possible presence of either a binary galactic core or a stellar mass that will eventually become the core. The outer regions of the galaxy appear diffuse.
