The galaxy presents an elliptical morphology. It appears to be relatively smooth in texture, with a high degree of central concentration of luminosity. The core region displays a bright, yellowish-white hue, indicating a population of older stars. The outer regions exhibit a gradual decrease in surface brightness, transitioning to a redder color suggesting an aging stellar population and a lower rate of recent star formation. A slight asymmetry is observed in the light distribution, with one side appearing slightly more extended than the other, although this could be due to tidal interactions. There is very little indication of dust lanes or spiral arm structures. The overall impression is that of a mature, relatively quiescent system.