The galaxy presents a generally smooth and rounded morphology. Its color profile is dominated by redder wavelengths, suggesting an older stellar population. There is no distinct spiral structure visible, but there is a potential very faint disk shape to it. The galaxy does not exhibit any major signs of ongoing merger activity or significant disturbances, instead appearing relatively undisturbed and well-defined. It shows an elliptical shape with a bright core. The galaxy's substantial size and luminosity imply a significant mass, likely dominated by older stars and potentially a supermassive black hole at its center. Overall, the galaxy appears to be a quiescent, evolved system with minimal current star formation.
