This galaxy appears to be a relatively massive system with a smooth morphology, likely an elliptical or lenticular type. The light distribution is concentrated, with a noticeable central bulge. The overall color appears relatively red, suggesting a population of older stars and a low rate of on-going star formation. There is a slight asymmetry, with one side being slightly elongated. There is no evidence of strong spiral arm structures or significant dust lanes. The galaxy could be potentially interacting with a smaller galaxy.
