The galaxy exhibits a morphology that suggests it is undergoing a significant interaction or disturbance. The overall form is irregular. There is possible evidence of tidal features, potentially faint and diffuse extensions that emanate from the main galactic body. These extensions could be indicative of gravitational interactions with another galaxy or object. The galaxy's structure appears complex, with asymmetries and potentially distorted spiral arm segments. There is an indication of clumpy star formation regions within the galaxy. These regions appear as localized concentrations of brighter, possibly bluer light. It is difficult to determine if the galaxy has a central bulge or a well-defined disk component. The inner region of the galaxy is relatively luminous, but its overall light distribution appears to be irregular.
