The galaxy presents as a fairly smooth, centrally concentrated object with a generally round morphology, though appearing slightly elongated. The central region exhibits a yellowish-orange hue, suggesting an older stellar population. The outer regions appear to have a bluer color, which could indicate the presence of younger, hotter stars and potentially some ongoing star formation, albeit at a low rate. There is a hint of some minor disturbance or faint tidal feature, but no strong indication of an ongoing major merger. The overall structure indicates the galaxy is most likely an elliptical galaxy in the process of a merger.
