The galaxy presents as a single, centrally concentrated object with a smooth, elliptical morphology. It exhibits a spheroidal shape, with minimal discernible structure beyond a general gradient in luminosity from core to periphery. There is no apparent disk component or spiral arm structure visible in this image. The color profile suggests an older stellar population, with a redder hue concentrated towards the core and a faint bluer halo. There is no obvious evidence of ongoing merger activity or significant tidal disturbances. The galaxy appears relatively undisturbed and quiescent. 
