The galaxy presents as a generally smooth and centrally concentrated object, exhibiting an elliptical morphology. It possesses a bright, yellowish core which gradually transitions into a more diffuse, blueish-white halo. There is little evidence of prominent spiral arm structures or distinct dust lanes. The overall appearance suggests a system dominated by an older stellar population, although some ongoing star formation may be present, inferred from the slight blueish hue. Minor disturbances are possibly hinted at within the outer regions of the halo, but the overall structure suggests a system that has undergone some level of past interaction. The galaxy appears to be reasonably massive based on its size and luminosity. Its shape is somewhat in between round and elongated.
