The galaxy exhibits a complex morphology, potentially indicative of an ongoing or recent merger event. One component presents as a relatively smooth, centrally concentrated spheroid with a yellowish-white hue. This suggests an older stellar population with limited ongoing star formation. The other component appears elongated, more diffuse, and displays a more prominent yellow to reddish color gradient, possibly due to dust obscuration or variations in stellar population age. The overall structure hints at gravitational interactions, though the precise nature and stage of the interaction are difficult to ascertain from the single image. The redshift of 0.129898 suggests that the galaxy is relatively distant.
