The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. Its color is predominantly bluish, indicating the presence of relatively young stellar populations. The galaxy exhibits a slight elongation, though it appears generally round. There is no visible evidence of spiral arms or significant dust lanes. The galaxy appears to be a relatively undisturbed system, showing minimal signs of recent mergers or tidal interactions. The central region displays a higher surface brightness, possibly indicating the presence of a dense stellar nucleus. The overall appearance suggests a relatively evolved system, potentially an elliptical or lenticular galaxy undergoing ongoing star formation at a moderate rate.
