This galaxy appears to be an elliptical galaxy with a smooth, featureless morphology. It presents as a well-defined, concentrated object with a high degree of central light concentration, and a relatively round shape. There is no visible evidence of spiral arms or a distinct disk structure. The light distribution suggests an older stellar population, likely dominated by Population II stars, which are typically found in elliptical galaxies. There's some indication of subtle color gradients within the galaxy, with the core potentially appearing slightly yellower/redder compared to the outer regions, which could imply variations in stellar populations and metallicity. No significant signs of ongoing or recent major merging events are apparent, with the overall structure suggesting a galaxy that has undergone substantial dynamical relaxation. There's a slight indication of a minor disturbance possibly from a small satellite galaxy. The apparent red color suggests that dust may be present, however the color is more likely due to an older stellar population.
