The galaxy presents as a concentrated, centrally-brightened system with a generally smooth morphology. The overall shape appears elliptical, deviating slightly from perfect circularity. There is a distinct color gradient, transitioning from a yellowish-white hue at the core to a reddish tinge in the outer regions. No spiral arms or distinct dust lanes are discernible. There is no apparent ongoing major merging event, although a slight asymmetry in the outer halo hints at a potential minor interaction or disturbance in the past. The overall color suggests a relatively evolved stellar population, with a lower ongoing star formation rate compared to younger, bluer galaxies.
