The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The light profile suggests a dominant bulge component with a gradual decrease in luminosity towards the outer regions. There is a subtle color gradient observable, transitioning from a slightly yellower core to a redder halo. No distinct spiral arms or prominent dust lanes are apparent. There are no signs of any major merging events or tidal disturbances that are readily visible. Based on the morphology alone, a classification as an elliptical galaxy is reasonable.
