This galaxy exhibits a moderate redshift, suggesting a significant distance. The light emitted from this galaxy has been stretched as it travels towards us. It appears to be a relatively massive galaxy with a notable star formation rate.  Based on its estimated size, it's a large galaxy. It has a complex morphology. While it presents a partially smooth appearance, there is evidence of more complex structures present. It shows signs of disturbances, possibly indicating an ongoing or recent interaction or merger event. It is uncertain what is causing the disturbance to this galaxy but it shows distinct signs of possible recent mergers. The color distribution suggests varying stellar populations, with the central regions displaying a reddish hue, potentially indicative of older stars, while the outskirts show bluer regions, which may indicate younger star formation. Further spectroscopic analysis would be necessary to confirm the stellar populations and kinematics.
