The galaxy presents a complex morphology, appearing to be in a late-stage merger or undergoing significant tidal disruption. The primary component is a bright, compact core, possibly indicative of a supermassive black hole or a dense stellar population. This core exhibits a distinct blue color, suggesting recent star formation. 

Extending outwards from the core is a prominent tidal tail or stream of material, which is yellowish-red. This feature suggests a gravitational interaction with another galaxy or a past merger event. The overall structure of the galaxy deviates significantly from a standard elliptical or spiral shape. There are no discernable spiral arms or a well-defined galactic disk. The redder color of the tail indicates an older stellar population within the tidal tail, with little ongoing star formation. The general appearance suggests that galaxy is experiencing a relatively high rate of star formation in comparison to similar galaxies.
