The galaxy appears to be composed of two distinct components. One component presents a more diffuse, bluish-white appearance, suggesting a higher proportion of younger, hotter stars. The other component exhibits a more concentrated, yellowish-orange hue, potentially indicating an older stellar population or significant dust obscuration. The overall morphology is somewhat irregular, with hints of gravitational disturbance. A possible merger or tidal interaction could be occurring, with each structure undergoing disruption, suggesting dynamical activity and potentially triggered star formation. The galaxy is estimated to be quite massive, although its current star formation rate is relatively low. 
