The galaxy presents an elliptical morphology, although exhibiting some disturbance in its structure, likely due to an ongoing merger event. Two distinct components are apparent: a more rounded, brighter, and bluer region to the east, and a somewhat elongated and yellower region to the west. The blue hue suggests active star formation within that region, while the yellower color of the other suggests an older stellar population with less ongoing star formation. There is evidence of interaction between the two components, potentially leading to the eventual coalescence of the two into a single galaxy.
