The galaxy presents as a relatively smooth, single structure with a slightly elongated morphology. The light distribution suggests a centrally concentrated spheroid, although a faint disk component cannot be entirely ruled out. The galaxy's color appears consistent across its extent, trending towards the redder end of the spectrum. There appears to be ongoing or recent galaxy interaction or possibly a full merger of multiple galaxies. It appears to be a merger in the final stages. There is a relatively high degree of symmetry and its shape appears to fall somewhere between round and elongated. It does not appear to be strongly disturbed or undergoing a major merger.
