The galaxy presents as a relatively smooth, centrally concentrated object with a noticeable spheroidal shape. The core region appears bright and yellowish, indicating a potentially older stellar population or significant dust obscuration. Moving outwards from the core, the light gradually fades into a more diffuse halo, exhibiting a bluer hue, suggesting the presence of younger stars or lower metallicity gas in the outer regions. There are no prominent spiral arms or distinct dust lanes visible. There is slight asymmetry. Based on its color and morphology, this galaxy is most likely an elliptical galaxy.
