This galaxy, at a redshift of approximately 0.22, exhibits a primarily smooth morphology. It is roughly elliptical in shape, and classified as a relatively rounded system. Light from the galaxy suggests two distinct, bright, yellowish central cores, possibly indicating an ongoing or recent merger event. There is visual evidence of distortion or tidal features, which further supports the hypothesis of a merging system. Based on its colors, it appears to contain a significant population of older stars, exhibiting a reduced rate of star formation and relatively low specific star formation. The system appears to be quite massive.
