The observed galaxy presents a complex and potentially disturbed morphology. A significant portion of the light appears concentrated in a bright, central region exhibiting a smooth profile, possibly indicative of a bulge component. Extending from this central region is a prominent, arcing structure. This arc presents a non-uniform distribution of light, suggesting the presence of spiral arm-like features. A significant disturbance is also observed. The shape is irregular and elongated. There's some evidence of ongoing or recent interaction with another galaxy.
