The galaxy presents as a fairly smooth, centrally concentrated object. Its overall shape is elliptical, exhibiting a somewhat elongated morphology rather than a perfectly circular one. The core is a bright yellow-white, indicating an older stellar population that is likely dominated by red giant stars. This central region appears to fade into a more diffuse halo. 

There is a hint of bluer light at the edges, suggesting some younger, hotter stars are present within what might be the outer disk, although distinct spiral arms are not observed. There is also some indication of minor disturbances, but overall the galaxy appears to be relatively undisturbed.
