The galaxy appears to be undergoing a significant merger event. There is a notable disturbance in the galaxy's structure. One part of the galaxy appears more concentrated and yellowish, possibly indicating an older stellar population. The other part shows bluer hues, hinting at ongoing or recent star formation. The overall form of the galaxy is distorted, lacking a well-defined spiral or elliptical shape. There are indications of tidal features or debris extending outward, supporting the conclusion that this galaxy has experienced a major interaction.
