This galaxy presents as a somewhat centrally condensed, luminous structure with a generally smooth appearance, and is observed to be at a redshift of z=0.22. It exhibits a shape that deviates slightly from a perfect circle, appearing somewhat rounded. There is visual evidence of two distinct bright centers, one brighter than the other, suggesting a possible ongoing or past interaction or merger event. The color profile indicates a redder hue in the galaxy's light, with a hint of green, which could be due to older stellar populations, or significant dust obscuration. The system shows some signs of disruption, but on the whole appears relatively unperturbed, with most classifications indicating that it does not present major disturbances or significant merging activity.
