This galaxy appears to be undergoing a merging event, or at the very least, exhibits signs of significant gravitational disturbance. There is an apparent core structure, but it is not well-defined, and shows a somewhat asymmetric profile. Faint wisps or tails are emanating from the central body, possibly tidal features resulting from gravitational interaction. There is a subtle color gradient across the galaxy, suggesting a slight difference in stellar populations or dust content in different regions. The overall light distribution is diffuse, indicative of extended stellar halos or tidal debris. There is no definitive disk structure visible. The galaxy has low surface brightness and seems relatively compact, but exhibits irregular morphology.
