The galaxy presents as a centrally concentrated system, approximately elliptical in shape. Its core exhibits a bright, nearly unresolved nucleus, suggesting the presence of a significant concentration of stars. The light profile transitions smoothly from this bright core to a more diffuse halo. While there are suggestions of disk-like structure, there are also signs of disturbances in the morphology. The color gradient from the center outwards shifts from yellow/white to bluish. This suggests a population of younger, bluer stars present away from the core, possibly indicating ongoing star formation. However, the generally smooth appearance indicates it is relatively evolved, with signs of a possible past merger event.
