The galaxy presents as a primarily smooth, centrally concentrated object with a near-circular morphology. The core exhibits a yellowish-orange hue, potentially indicating an older stellar population or significant dust obscuration. A faint greenish-blue halo surrounds the central region, suggesting the presence of a younger stellar population or ongoing, low-level star formation activity within the galactic disk or outer regions. There is no prominent disk structure or spiral arm features visible in the image. There's no obvious signs of tidal interactions or significant morphological disturbances, suggesting that it has not undergone a recent major merger. The galaxy appears relatively isolated and undisturbed.
