The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light profile with a high degree of symmetry. Its morphology suggests a relatively evolved system with little evidence of spiral arms or significant disk structure. The galaxy displays a mostly featureless morphology with a slight deviation from a perfect circle, with no cigar shape. The color gradient indicates a concentration of older stellar populations in the central regions, gradually transitioning to a somewhat bluer outer halo, suggesting possible ongoing low-level star formation activity or the presence of younger stars in the outskirts. The overall color is fairly red, indicating that it is mostly composed of older stars. There are no clear signs of a major ongoing merger, although the possibility of past minor interactions or disturbances cannot be ruled out given some subtle irregularities in the outer regions of the galaxy. 
