The galaxy presents a largely smooth, elliptical morphology. The light distribution appears centrally concentrated with a diffuse, extended halo. The core region exhibits a yellowish-orange hue, suggesting an older stellar population, and there is no apparent dust lane or spiral arm structure visible. The galaxy displays a high degree of roundness. There are no signs of tidal disturbances or ongoing mergers. The observed color gradient suggests that the outer regions are slightly bluer compared to the core. Overall, the galaxy is characterized by its relatively quiescent state and old stellar population.
