The galaxy exhibits a morphology indicative of a merger event, possibly involving multiple interacting components. There appears to be two dominant galactic bodies, potentially elliptical galaxies, in the process of merging.  A tidal bridge of material appears to connect the two larger objects.  The overall shape is irregular and disturbed, lacking any clear spiral structure or a defined central bulge in at least one of the objects.  There may be an additional compact object within the system.  Some dusty structures might be forming due to the merger. The system's color profile suggests a mix of older stellar populations (redder hues) and regions of recent star formation (bluer hues), concentrated in what could be spiral arm remnants in at least one object. The overall light distribution is complex and uneven, typical of interacting galaxies undergoing significant dynamical disturbances.
