The galaxy exhibits a morphology suggesting an ongoing interaction or merger. The main body appears somewhat smooth, although with some irregularities. A tidal tail or distorted arm is observed extending from the central region. The color distribution indicates a complex stellar population, with a central yellowish-white concentration suggesting older stars, surrounded by a bluish halo which is potentially indicating regions of recent star formation. The structure also appears slightly elliptical, but potentially disrupted by ongoing interactions with other objects. 
