The galaxy presents as a relatively smooth, centrally concentrated object. It is generally elliptical in appearance, with a slightly elongated shape. The core of the galaxy exhibits a yellowish-white color, suggesting a population of older stars. A subtle transition to a bluish hue is noticeable in the outer regions, perhaps indicating the presence of a younger stellar population or some star formation. There are no readily apparent spiral arms or a distinct disk structure, although a subtle flattening can be observed. The overall structure appears undisturbed, without any signs of major mergers or tidal distortions. Faint asymmetries or minor disturbances may be present but the galaxy seems to be in a relatively relaxed state.
