The galaxy presents as a centrally concentrated object with a roughly elliptical morphology. There is a smooth, diffuse halo surrounding a brighter, more compact central region. The color gradient suggests a blue central region, potentially indicating ongoing or recent star formation. The outer halo appears redder, which might be indicative of an older stellar population. There's no evidence of spiral arms or a well-defined disk structure, although the lack of morphological disturbance would indicate that the galaxy has not undergone a recent major merger event. Overall, based on the image, it appears to be a relatively undisturbed, early-type galaxy with some residual star formation.