The galaxy appears to be an elliptical galaxy, elongated in shape, and oriented at an angle relative to our line of sight. It exhibits a smooth, featureless profile with a bright, concentrated core that gradually fades into the surrounding halo. The color gradient suggests a dominant population of older stars. There are no distinct spiral arms or dust lanes visible. There's no apparent major merger activity. The galaxy appears relatively isolated and undisturbed. There is a slight reddish tint to the outer regions, and appears to be undergoing relatively low rates of star formation.
