The galaxy presents an elliptical morphology, appearing smooth and relatively featureless at this resolution. The light distribution is concentrated towards the center, with a gradual decrease in intensity outwards. The galaxy exhibits a color gradient, with the central region appearing more yellowish-white, possibly indicating an older stellar population, whereas the outer parts have more of a greenish tint which might suggest younger stars. A minor disturbance, possibly related to tidal effects, is suspected. No spiral arms or significant dust lanes are apparent. Overall, the galaxy seems to be undergoing a rather quiescent phase of stellar evolution.
