The galaxy presents as a disturbed system, appearing to be in the process of a significant merger.  The morphology is complex and irregular, with a dominant central region exhibiting a diffuse, amorphous structure.  There is a primary, more well-defined central component with a yellowish hue, which appears to be the core of one of the merging galaxies.  Faint, bluish extensions emanate from this core, suggestive of tidal tails formed during the interaction.  

A secondary, less-defined luminous region is also visible, suggesting another galactic nucleus involved in the merger.  This region exhibits similar blueish tidal features that connect to the dominant galaxy.  Dust lanes and/or enhanced star formation regions are suspected, hinted at by the diffuse nature and color variations within the interaction. Overall, the galaxy is dominated by the interaction and exhibits features indicative of ongoing gravitational disturbance.
