The galaxy appears to be of elliptical morphology, with a smooth, centrally concentrated light profile. The core is characterized by a strong yellowish hue, gradually transitioning to a greenish halo. The isophotes are generally circular, with minimal indication of spiral arms or other distinct features. There is no obvious dust lane or tidal disturbance present, suggesting it is a relatively undisturbed system. There is a slight variation in luminosity radiating from the center, with the core appearing more tightly concentrated. The outer regions exhibit a fainter and more diffuse emission, fading into the background. The overall color distribution suggests a stellar population with a relatively large population of older stars.
