The galaxy presents a generally smooth morphology. It appears to be undergoing a significant merger event. Two distinct nuclei are visible within the galaxy's central region, indicating an advanced stage of the interaction between the two progenitor galaxies. The overall shape is somewhat rounded but noticeably disturbed, showing tidal features that suggest gravitational interactions. There's a subtle asymmetry and faint, extended structures that could be tidal tails or debris from the merging process. The color distribution indicates a mix of stellar populations, with a concentration of older, redder stars. The presence of what appears to be bluer regions interspersed with the older population suggest some amount of on-going star formation.
