The galaxy appears to be relatively compact, exhibiting a disturbed morphology. The central region displays a concentrated area of bright emission, exhibiting a clumpy structure with a hint of multi-color emission. There are some faint wispy extensions suggestive of tidal debris. The core is surrounded by a more diffuse and lower surface brightness component. There is a faint hint of blue color in some parts of the galaxy, potentially indicative of recent star formation. There seems to be an ongoing interaction or recent merger event, based on the asymmetry of the shape. Overall, the galaxy is an interacting system displaying signs of tidal disruption.
