The galaxy presents as an elliptical morphology, elongated along its major axis. The central region exhibits a brighter, concentrated luminosity, potentially indicating a significant stellar population and/or a central supermassive black hole. The outer regions appear fainter and smoother, suggesting a decrease in stellar density with increasing radius. 

There is a subtle color gradient visible, with a slightly bluer hue toward the central region, possibly indicating younger, hotter stars. The outer regions appear redder, which may be indicative of an older stellar population. The galaxy appears relatively undisturbed with a smooth, regular structure. There are no obvious signs of spiral arms, dust lanes, or tidal features. The galaxy's light is redshifted. 
