The galaxy presents as a relatively smooth, centrally concentrated object with an apparent radial symmetry. It exhibits a color gradient, transitioning from a yellowish-white core to a bluer, more diffuse outer region. There is a slight elongation to its shape, deviating from a perfectly circular morphology. No distinct spiral arms or a prominent disk are visible. The general appearance suggests a mature system with ongoing, albeit possibly moderate, star formation. There is a hint of possible disturbance of it's shape, but no obvious signs of on going or recent major mergers.
