The galaxy appears as an elongated, irregular structure. There is evidence of a possible interaction or merger occurring. A primary, elongated component is visible, displaying a smoother, more diffuse light profile, possibly indicative of an older stellar population. There is a secondary component that appears more compact and has a warmer colour. The overall colour suggests the presence of both older and younger stellar populations within the system. The galaxy exhibits features that deviate significantly from a regular elliptical or spiral morphology.
