The galaxy presents as a largely featureless, elliptical or spheroidal structure. It exhibits a high degree of central concentration with a smooth and rounded light distribution, indicating an older stellar population. The core region displays a yellow-white hue, suggesting a population of evolved stars with low star formation. Fainter red hues are visible in the outer regions, which is also indicative of an older stellar population. There is no apparent disk or spiral arm structure visible. No significant tidal distortions or merger signatures are discernible, though there may be a very minor disturbance in the lower right of the image. The overall impression is of a relatively undisturbed and evolved galaxy.
