The galaxy appears as a luminous, centrally concentrated object. Its morphology is generally smooth and elliptical in shape, with a high degree of roundness. There is minimal evidence of spiral arms or significant disk-like features. The light distribution suggests an older stellar population, consistent with a quiescent galaxy where active star formation is suppressed. There's a slight indication of disturbance on the galaxy's edges, but these are mild, and no major merging or tidal features are obvious. Overall, the galaxy is a massive, red-sequence system with little current star formation.
