The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. A bright, yellowish core dominates the galaxy's center. This core gradually fades into a surrounding diffuse halo, exhibiting a bluer hue than the central region. The bluer color of the halo might indicate the presence of a younger stellar population compared to the core. The overall structure suggests a relatively evolved system, potentially an elliptical galaxy, with minimal evidence of ongoing merger activity or significant star formation.
