The galaxy presents an overall elliptical morphology, appearing largely smooth and featureless. Its color profile exhibits a central reddish hue, gradually transitioning to a greenish-blue periphery. This color gradient suggests a centrally concentrated older stellar population with ongoing star formation in the outer regions. There is no obvious evidence of a galactic disk. The galaxy appears relatively undisturbed, showing no signs of major mergers or tidal disruptions. It may be undergoing some form of minor interaction, but there is no strong indication of significant recent merging activity. 
