The galaxy appears to be undergoing a significant interaction or merger with another galaxy. One primary component displays a relatively smooth, elliptical morphology with a dominant yellowish-orange hue, suggesting a population of older stars and lower levels of active star formation. The other component appears more compact and bluer in color, indicative of younger stellar populations and potentially higher rates of star formation. There is noticeable tidal disruption, with faint extensions or tails emanating from the interacting galaxies. There is a hint of disturbed morphology in the primary body, possibly caused by gravitational interaction. The overall system appears to be undergoing significant dynamical evolution.
