The galaxy presents as a centrally concentrated system, exhibiting a smooth, elliptical morphology. The core region displays a distinct yellowish-orange hue, suggesting a population of older stars or significant dust obscuration. A more diffuse, bluish halo surrounds the core, potentially indicating the presence of a younger stellar population or ongoing star formation, albeit at a low rate. There is no clear evidence of spiral arms or a distinct disk structure. The galaxy appears largely undisturbed, with no signs of major mergers or significant tidal interactions, though a minor disturbance cannot be ruled out. Overall, the galaxy appears to be a relatively massive, evolved system.
