The galaxy presents a generally smooth, elliptical morphology. The light distribution appears centrally concentrated with a gradual decrease in intensity towards the outer edges. The color is relatively uniform across the galaxy, with a slight tendency towards redder hues. There is no apparent structure such as spiral arms, bars, or dust lanes. The overall appearance suggests an evolved stellar population, consistent with a galaxy that has largely ceased active star formation. There are no signs of tidal interactions or major disturbances, indicating relative isolation and stability. 
