The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears elliptical, with a high degree of roundness and limited discernible disk-like features. The galaxy exhibits a distinct color gradient, transitioning from a bright, yellowish-white core to a fainter, reddish-orange halo. There are no obvious signs of active merging events or major disturbances in the galaxy's structure. The overall impression is that of a quiescent galaxy with a dominant, older stellar population.
