The galaxy appears to be undergoing a significant interaction or merger. There are two distinct luminous components visible. The primary component exhibits an elongated, irregular morphology, with evidence of tidal features or distortions suggesting a gravitational interaction. This component shows a bluish tint, potentially indicating regions of active star formation. The secondary component is more compact and has a yellowish hue, suggesting an older stellar population and potentially a more spheroidal morphology. The overall structure is complex, lacking a clear disk or spiral arm pattern. The system appears to be in an advanced stage of merging. Based on color, the star formation rate of the galaxy appears relatively low.
