This galaxy exhibits a complex morphology, appearing to be in a state of interaction or recent merger. The system is characterized by a dominant, moderately luminous, central component which is relatively smooth in appearance. Extending outward from this central region are faint tidal features or tails, suggesting gravitational disturbance and interaction with another galactic body. These features show lower surface brightness compared to the core. The elongation and disrupted shape indicate this galaxy may be classified as an intermediate-type spiral galaxy. The color distribution suggests a mix of older stellar populations and recent star formation, with bluer regions potentially indicating ongoing or recent starburst activity. The overall light distribution is not perfectly symmetrical, further supporting the disturbed nature of the galaxy.
