The galaxy presents as a relatively smooth, centrally concentrated object. There is a noticeable color gradient, transitioning from a yellowish core to a redder outer halo. While the galaxy appears mostly featureless, a faint suggestion of a disk-like structure may be present upon closer inspection. The galaxy exhibits a high degree of circular symmetry, suggesting a minimal disturbance from recent merger activity. It appears to be a mature system with a notable population of older stars in its central region.
