The galaxy presents a largely smooth, elliptical morphology, appearing round with minimal visible disk-like structure or spiral arms. A small fraction of disturbances might be present, but the galaxy overall looks undisturbed. Color gradients show a slight reddening towards the core suggesting an older stellar population concentrated centrally, with bluer hues potentially arising from younger stars or ongoing star formation in the outer regions. This is reinforced by the estimated mass and star formation rates, which indicate moderate mass and relatively low ongoing star formation activity.
