The galaxy appears as a centrally concentrated, relatively smooth elliptical system. There is little evidence of spiral arms or a significant disk component. The galaxy's light profile suggests a spheroid-dominated morphology. The overall color is yellowish, which could be due to an older stellar population. There is no apparent ongoing major merger activity or tidal features, although it is possible there are very minor disturbances visible. The galaxy appears quite large, with a significant effective radius.
