This galaxy exhibits a generally smooth morphology, with a centrally concentrated light profile. The shape appears mostly round, deviating slightly from perfect circularity. There is evidence of a possible interaction or merging event. The main body of the galaxy appears relatively undisturbed, but there is a clear irregularity or additional component adjacent to it which could be another galaxy. There are no obvious spiral arm structures or a well-defined disk component visible. The colour gradient is subtle; it appears yellower near its core and slightly bluer in the outskirts, suggestive of a population of older stars in the core and some younger stars in the outer regions.
