The galaxy appears to be an elliptical type, exhibiting a smooth, relatively featureless morphology. The light profile suggests a centrally concentrated distribution of stars, with brightness decreasing gradually towards the outer edges. The galaxy exhibits a shape somewhere between round and oblong. There is a very slight blue tint on the outer edges, which suggests a low amount of recent star formation. There are no apparent signs of spiral arms, dust lanes, or significant tidal disturbances, indicating a well-mixed stellar population and a lack of ongoing major mergers.
