The galaxy presents a morphology suggestive of an ongoing or recent merger event. Two distinct, luminous cores are visible, indicating the presence of two progenitor galaxies interacting gravitationally. The overall shape is disturbed, lacking a clear spiral or elliptical structure. A bridge of material appears to connect the two primary cores, possibly representing tidal debris or star formation triggered by the interaction. The color gradient suggests a range of stellar populations, with yellower hues concentrated in the central regions, and a more diffuse blue component in the surrounding areas, potentially indicating active star formation. The system appears relatively compact, with no extended tidal tails readily discernible in this image.
