The galaxy presents a generally smooth morphology. The light distribution appears centrally concentrated, with a gradual decrease in intensity towards the outer regions, presenting an elliptical shape with some indication of a flattened form. The core displays a distinct yellow-white hue suggesting an older stellar population. Fainter, reddish tinges may indicate possible recent star formation in some regions, but it appears to be limited. There is no discernible spiral arm structure or prominent dust lanes visible. The overall appearance suggests a mature system with a likely high mass. It appears largely undisturbed, with no obvious signs of major interactions or mergers.
