The galaxy appears to be an elliptical or lenticular type. It exhibits a smooth, centrally concentrated morphology with a high degree of roundness, and it is approximately 9 kiloparsecs in diameter. The galaxy displays a color gradient, with a yellowish-white core, suggesting an older stellar population dominating the central region. The outer regions appear slightly bluer, possibly indicating the presence of a younger, albeit subdued, stellar population, meaning the galaxy may still be forming stars, though at a slower rate. There is no discernible evidence of spiral arms or a bar structure, and there are no signs of ongoing major mergers or significant tidal disturbances. The galaxy exhibits no discernible morphological features beyond a slightly blurred, smooth, centrally concentrated light distribution, indicating the absence of significant star-forming regions, or dust lanes.
