The galaxy presents as a centrally concentrated object with a relatively smooth morphology. The light profile appears mostly uniform, fading gradually from the center without strong spiral arm structures or prominent knots of star formation visible in this color image. The color gradient suggests a possible redder core region transitioning to a slightly bluer halo, indicative of a potential difference in stellar populations. Its overall shape is closer to round than elongated or disk-like. The smoothness and color suggest an elliptical-like morphology. There is no obvious evidence of ongoing major mergers or significant tidal disturbances in this image.
