The galaxy presents as a centrally concentrated, smooth object. It is likely an elliptical galaxy, as evidenced by its generally featureless appearance and high degree of central concentration. The galaxy has a moderate degree of ellipticity. The color gradients suggest an aging stellar population, with the central region displaying a more yellow-red hue, potentially indicating a higher concentration of older stars, while the outer regions appear bluer. There does not appear to be any evidence of significant ongoing star formation. There are no obvious signs of tidal disturbances or recent merger activity.
