The galaxy presents a generally smooth, elliptical morphology. The light distribution suggests a centrally concentrated spheroid. Its overall shape is elongated, displaying an axial ratio suggesting it is not perfectly spherical. There is no obvious spiral structure present. 

The color gradient indicates a redder core, potentially indicative of an older stellar population, with bluer hues visible in the outer regions, perhaps due to more recent star formation, though this is subtle. There is little evidence of significant dust lanes or other obscuring material. No signs of major tidal disturbances or ongoing mergers are immediately apparent in the image.
