The galaxy appears to be an elliptical galaxy, exhibiting a smooth, featureless morphology without discernible spiral arms or a prominent disk. Its overall shape is generally rounded. A slight elongation is observed, suggesting it is not perfectly spherical, but rather somewhat flattened. The luminosity distribution appears centrally concentrated, with a bright core that gradually diminishes outwards. The galaxy's color indices suggest a population of older stars. There is no obvious evidence of recent major mergers or significant tidal disturbances in the surrounding environment. However, a minor disturbance cannot be ruled out.
