The galaxy presents a morphology suggestive of an ongoing or recent merger. A distinct, brighter central region is visible, indicating a high concentration of stellar mass, likely the original core of one of the merging galaxies. There appears to be an additional, smaller concentration of luminosity situated nearby, indicative of a secondary core. The overall color of the system leans towards the redder end of the spectrum, possibly indicating an older stellar population. There is evidence of tidal distortion, as faint streams of light can be seen emanating from the main body of the galaxy. These streams are most likely composed of stars and gas stripped from the progenitor galaxies during the interaction. The overall shape is amorphous, lacking any clear spiral or elliptical structure.
