The galaxy presents as a primarily smooth, elliptical structure with an apparent roundness, although it exhibits slight deviations from a perfect circular shape, potentially due to its in-between roundness class. The core of the galaxy displays a concentrated, yellowish hue, which may indicate an older stellar population. Moving outwards from the center, the galaxy appears to fade into a reddish halo or extended, tenuous disk, suggesting the presence of older stars. This galaxy does not show any indications of major mergers. There are no prominent spiral arms or distinct morphological features within the galaxy. Star formation appears to be minimal.