The galaxy presents as an interacting system, possibly in the late stages of a merger. The primary component exhibits a largely smooth morphology, suggestive of an elliptical galaxy. Its color is generally white, hinting at an older stellar population with little ongoing star formation. A secondary component is evident, showing a distinctly irregular shape and a bluer hue. The blue color indicates the presence of younger, hotter stars and recent or ongoing star formation. The two components appear to be gravitationally bound, with tidal features perhaps present, though not clearly defined within the resolution of the image. The overall system appears somewhat compact. Further spectroscopic analysis would be valuable in determining radial velocities and confirming the merger scenario.
