The galaxy presents as a relatively smooth, centrally concentrated structure. Its overall form appears largely elliptical, exhibiting high degree of circularity. The central region displays a distinct yellowish hue, suggestive of an older stellar population. Progressing outwards from the core, a subtle transition to a bluer color is observed, implying the presence of younger stars in the outer regions. There is a hint of minor asymmetry in the galaxy's outer regions, with possibly a very faint indication of a disk, but this is difficult to discern from this image. There is no strong evidence of significant ongoing star formation or active galactic nuclei activity, given the lack of intense, localized emission regions or strong color gradients. The overall morphology suggests a galaxy that is relatively evolved, possibly undergoing a phase of quiescent evolution. The estimated size is likely between 3 and 4 kiloparsecs across.
