The galaxy presents as a merging system, exhibiting clear signs of gravitational interaction. Two distinct components are visible. The primary component appears round and smooth in morphology, with a concentrated central region. The secondary component is more elongated and less defined, possibly a smaller galaxy in the process of being tidally disrupted. The color gradient suggests ongoing star formation, particularly in regions where the two galaxies interact. The overall structure indicates a late-stage merger event, with significant tidal distortion present. Further spectroscopic analysis is recommended to determine the stellar populations and merger dynamics of this system.
