The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth, diffuse morphology. There is a notable lack of distinct spiral arms or significant dust lanes. The color gradient suggests a population of older stars, exhibiting a yellowish-white hue in the central region. The outer regions appear slightly bluer. Overall, there is no obvious indication of active star formation. The object has an angular size that is neither particularly small nor large, relative to other galaxies in the image. There are no signs of tidal features or significant disturbances that would indicate a recent major merger event, though a very minor interaction cannot be entirely ruled out.
