The galaxy presents a smooth, elliptical morphology. It exhibits a concentrated central bulge, suggesting a relatively old stellar population and minimal ongoing star formation. The color appears to be generally redder in the central regions and slightly bluer towards the outskirts, indicative of varying stellar populations and potential recent star formation in the outer regions. There is no evidence of spiral arms or a distinct disk structure. The overall shape is quite round and undisturbed. There is no apparent ongoing merger activity, nor any major tidal disturbances.
