The galaxy exhibits characteristics of a late-stage merger. The primary body displays a disturbed morphology, with evidence of tidal features and disrupted spiral arms. The central region is characterized by a bright, concentrated core, possibly indicative of active galactic nuclei activity or a high concentration of stars. The overall shape is amorphous with a noticeable extension indicating the presence of tidal tails. The color gradient suggests a mix of stellar populations, with bluer regions potentially indicating active star formation. The lack of a well-defined disk structure further supports its classification as a merging system.
