The galaxy presents as a luminous, relatively smooth object with a centrally concentrated light profile. Its overall morphology is elliptical, exhibiting a high degree of roundness. The central region shows a distinct yellowish-orange hue, potentially indicating a population of older stars and/or significant dust obscuration. A diffuse greenish halo surrounds the core, possibly indicative of a fainter, more extended stellar population or ongoing, albeit low-level, star formation. No distinct spiral arms or significant morphological disturbances are evident. The galaxy appears largely undisturbed, showing no major signs of interaction with other galaxies.
