The galaxy exhibits a complex morphology, appearing disturbed and likely undergoing a merging event. The primary body is a relatively smooth, elliptical-like structure with a concentrated core. A distinct tidal tail or plume-like extension is observed emanating from the main body, possibly indicating gravitational interaction with another galaxy. Patches of star formation are visible, particularly in the core and along the tidal feature, as indicated by the blueish hue. A notable portion of the overall light distribution displays redder colors suggesting an older stellar population. Based on its red shift, this object lies at a considerable distance. The absolute magnitude shows it is a luminous galaxy, despite low star forming activity.
