The galaxy appears as a centrally concentrated, largely homogenous object with a smooth light distribution. It is spheroidal in shape, showing a high degree of circularity. The galaxy exhibits a color gradient, transitioning from a reddish hue towards the core to a greenish-blue tinge in the outer regions. There is no obvious indication of spiral arms or a prominent disk structure. Minor disturbances or signs of ongoing mergers are not readily apparent from its morphology, indicating it is likely an isolated galaxy.
