This galaxy appears to be undergoing a significant interaction or merger. The morphology is disturbed, with a distorted overall shape. Two distinct luminous regions are visible. One region presents a reddish-yellow hue and the other a blueish color, suggesting differing stellar populations, with younger, hotter stars dominating the bluish region and older populations within the reddish-yellow area. Evidence of tidal tails or bridges is subtle but potentially present, indicative of gravitational interactions between galactic components. Star formation activity is likely present, particularly within the bluer region. The system shows a degree of asymmetry, reinforcing the interpretation of an ongoing merger. The overall light distribution suggests a moderately massive system.
