The galaxy presents a generally smooth and elliptical morphology. It appears to be a relatively compact system with a central bulge that is slightly elongated, with a ratio of major to minor axis not far from unity. The light distribution suggests a fairly well-mixed stellar population, with a subtle colour gradient. The galactic center is distinctly yellowish, possibly indicating an older stellar population, while the outer regions display bluer tones, hinting at the presence of younger stars or ongoing star formation, although at a relatively low rate. There is no clear evidence of spiral arms or any significant tidal disturbances. The overall structure points towards an evolved galaxy, potentially in the process of transitioning or having already transitioned to a more quiescent state.
