The object appears to be a galaxy at intermediate redshift. It presents as a disturbed system, possibly undergoing a merger or close interaction. There is a dominant, relatively smooth component with a yellowish hue suggesting an older stellar population. This primary component is closely associated with a smaller, bluer region, hinting at ongoing star formation. The overall morphology is irregular, with tidal features or asymmetries possibly present, but spatial resolution limits detailed analysis of these features. The system's luminosity appears significant, indicative of a massive galaxy with ongoing or recent star formation activity.
