The galaxy presents a morphology suggesting an elliptical or lenticular type. It exhibits a relatively smooth light distribution, with a central concentration that fades outwards. The shape is elongated, appearing somewhat flattened. There is no apparent spiral structure or prominent dust lanes. The color gradient suggests a population of older stars dominating the galaxy's composition, although a bluer hue indicates a small amount of recent star formation. Overall, the galaxy appears to be a relatively quiescent system.
