The galaxy presents as a relatively smooth, centrally concentrated object. It has a generally elliptical morphology with a round appearance. The color profile indicates a dominant population of older stars, with a yellowish hue concentrated in the core region. Fainter, diffuse light extends outwards from the core, creating a surrounding halo. There is no obvious presence of spiral arms, distinct dust lanes, or major star-forming regions. The overall structure suggests a system that has largely completed its major mergers and is now in a relatively quiescent state. Minor disturbances or interactions cannot be entirely ruled out, though no distinct features are readily observable in the image.
