The galaxy exhibits a morphology suggestive of an ongoing or recent merger event. Two distinct, roughly spherical, luminous components are observed. One component appears redder in color, potentially indicating an older stellar population or significant dust obscuration. The other component has a more yellow-orange hue, hinting at a younger stellar population or less dust. There is some indication of tidal features or disturbed morphology surrounding the two components, though the limited resolution makes detailed analysis challenging. The overall light distribution appears relatively smooth, suggesting a system that is transitioning toward a more relaxed state after the initial merger. Based on the color indices, this galaxy is likely a massive system with ongoing, though potentially subdued, star formation. The system exhibits a generally rounded appearance. There is significant disturbance in the center of the galaxy, possibly related to a previous or ongoing merger event.
