The galaxy presents a predominantly smooth morphology, appearing as an elliptical system with a subtle blue hue concentrated towards the center. This central coloration might indicate the presence of a younger stellar population or a region of ongoing star formation, albeit at a relatively low rate. The shape is best described as moderately rounded, displaying a slight elongation but lacking any pronounced disc-like structure. There is a faint suggestion of a minor disturbance in the form of a slight asymmetry or faint tidal tail, possibly indicative of a past interaction or merger event. Overall, the galaxy appears as a relatively small and low-mass system, possibly in transition from a more actively star-forming state to a quiescent one.
