The galaxy presents as a centrally concentrated object with a roughly elliptical morphology. The core exhibits a strong, yellowish luminosity, suggesting a significant population of older stars. Extending outwards from the core, a less luminous and slightly bluer halo can be observed. This suggests the presence of a younger stellar population within a relatively compact disk or extended structure. The galaxy displays a smooth appearance, lacking prominent spiral arms or significant dust lane features, supporting a relatively passive or undisturbed evolutionary history. Some minor asymmetry or subtle features may indicate minor interactions or disturbances.