The galaxy presents a generally smooth, elliptical morphology. It appears centrally concentrated, with a gradual decrease in luminosity from the core outwards. There is no strong evidence of spiral arms or a prominent disk structure. The color is generally yellow-white, suggesting an older stellar population with relatively little ongoing star formation. There are no distinct dust lanes or prominent star-forming regions visible. Based on its overall structure and color, it can be considered a very massive galaxy that is not undergoing any merging events.
