The galaxy appears to be a relatively smooth, centrally concentrated object. The core exhibits a bright, yellowish hue, suggesting a significant population of older stars. There is a diffuse, slightly elongated halo surrounding the core, exhibiting a subtle gradient in color and luminosity. No distinct spiral arms or bar structures are discernible. There are no obvious signs of recent major merger events or tidal disturbances in the image, although the subtle asymmetry could indicate minor interactions. Overall, the morphology is consistent with an elliptical galaxy or a lenticular galaxy seen at a relatively large distance.
