The galaxy presents as a centrally concentrated elliptical morphology. It exhibits a smooth, largely featureless appearance, lacking prominent spiral arms or a well-defined disk structure. The light distribution is highly concentrated towards the center, with a gradual decrease in surface brightness outwards. The core region appears yellowish, suggesting an older stellar population, while the outer regions show a slightly bluer hue, possibly indicative of some ongoing, albeit limited, star formation. There might be very minor disturbances in the structure, possibly indicating a past interaction or merger event, though these are not prominent. The galaxy does not show any signs of a strong bar structure or distinct rings. Overall, it seems to be a fairly evolved system.
