The galaxy presents as a centrally concentrated, ellipsoidal structure. The core exhibits a bright, yellowish-white hue, suggesting a significant population of older stars. Moving outwards from the core, the light becomes more diffuse with a subtle color gradient, indicating a mixture of stellar populations. The galaxy appears relatively smooth in texture, with only minor disturbances observed, indicating it is not currently undergoing any major merging events. The overall morphology points toward an elliptical or lenticular galaxy type, seemingly lacking prominent spiral arms or significant star formation activity.
