The galaxy presents as a relatively smooth, rounded structure with a notable concentration of light towards its center. The morphology indicates a high degree of central symmetry. A slight color gradient is observed, transitioning from a more yellowish hue at the core to a subtly bluer periphery. There is no discernible spiral arm structure or significant dust lane presence visible within the limitations of image resolution. The overall impression is consistent with an elliptical galaxy or a lenticular galaxy with a dominant bulge component. There are no major disturbances or signs of merging events visible.
