The galaxy presents as a disturbed system, exhibiting characteristics suggestive of a possible ongoing or recent merger event. The morphology is irregular with extended features that may be tidal tails or disrupted spiral arms, indicating gravitational interactions. There's a blend of colors across the galaxy, with the central region appearing more yellow, possibly indicating an older stellar population or dust obscuration. Fainter regions extend outward from the central bulk, these regions show hints of blueish hues, which might point to younger star formation activity. The overall appearance suggests a galaxy with a substantial stellar mass and a detectable rate of star formation despite its disturbed state. The asymmetry and irregular features are primary indicators that this galaxy is not in a state of equilibrium.
