The galaxy presents as a single, concentrated spheroid of light, with a smooth profile and no apparent substructure, such as spiral arms or a bar. The central region exhibits a yellowish hue, possibly indicating an older stellar population or a significant dust component obscuring bluer wavelengths. Surrounding this central area is a fainter, more diffuse halo, with a slight greenish tint on its periphery. The general roundness of the galaxy suggests a classification towards elliptical, with only very minor deviations from perfect circularity. There is no evidence of tidal tails or morphological distortions indicative of recent major merger activity, but some very subtle disturbances cannot be ruled out. The galaxy's color gradient, from yellow in the core to greenish in the outer regions, could imply variations in stellar population or dust extinction as a function of radius.
