The galaxy presents as an elliptical morphology, with a smooth and largely featureless appearance. The light distribution suggests a centrally concentrated spheroid. The core region exhibits a yellowish-orange hue, potentially indicating an older stellar population and/or dust obscuration. Moving outward from the core, the galaxy transitions to a bluer color, potentially representing the presence of a younger stellar population. There is no obvious spiral arm structure or prominent dust lanes visible in this image. Overall, the galaxy appears relatively undisturbed, lacking significant signs of tidal interactions or ongoing mergers, although slight disturbances cannot be ruled out at this resolution.
