The galaxy presents a largely smooth and elliptical morphology. The central region exhibits a high degree of concentration, appearing nearly spherical and bright. The color gradients suggest a relatively evolved stellar population, with a redder hue towards the outer regions. Faint disk-like structures may exist but are not highly pronounced. The general morphology shows evidence for minimal merging or tidal disturbances, indicating relative dynamical stability. Star formation appears present, but quiescent. The overall structure indicates a relatively massive system.
