The galaxy appears to be composed of two distinct components. One component presents as a spheroidal, relatively smooth and centrally concentrated structure, exhibiting a bluish hue suggesting recent or ongoing star formation. The other component appears more diffuse and elongated, displaying a reddish-orange color which could be attributed to an older stellar population or significant dust obscuration. There is no visible spiral structure or obvious signs of tidal disturbance. Based on its morphology it appears as a relatively massive galaxy.
