The object appears to be a galaxy undergoing a significant merger. There are multiple distinct luminous cores, indicative of multiple galactic nuclei in close proximity. The overall morphology is irregular and disturbed, lacking a well-defined spiral structure or elliptical shape. The dominant color is a yellowish-white, with some indication of redder hues, likely representing an older stellar population. Evidence of tidal tails or other merger remnants is subtle but potentially present. The object is relatively compact with a high central concentration.
