The galaxy presents a morphology dominated by smoothness. It appears largely spheroidal in shape, with a high degree of central concentration. A possible faint disk feature may be present, but is difficult to resolve. The light distribution exhibits a centrally bright, yellow-orange core, transitioning to a slightly bluer and dimmer outer halo. This suggests a possible mixture of stellar populations, with older stars concentrated in the central region.

The galaxy may be undergoing, or have recently undergone a merger event. Though the galaxy is mostly smooth, there appears to be some degree of disturbance to its main structure.
