The galaxy presents an amorphous morphology. It is dominated by a central bulge region exhibiting a yellow-orange hue, indicative of an older stellar population. A faint, diffuse structure extends outwards from this central region, displaying a bluish-white color. This extended feature might indicate a faint disk or tidal debris. There is a notable disturbance in the morphology, possibly hinting at a past or ongoing interaction or merger event. A substantial portion of the overall structure is amorphous, and a potential redder clump or region exists. There is no defined spiral structure is apparent.
