The galaxy presents a complex morphology, appearing to be a potential interacting system. It exhibits two distinct components: a more compact, brighter core region and a long, tidal feature extending from this core. The core displays a yellowish hue, possibly indicating an older stellar population. The tidal feature is elongated and fainter, suggesting material stripped from the main galaxy. The system's overall structure indicates a significant gravitational interaction or recent merger event. Based on visual assessment, the galaxy seems to show signs of disturbance from a possible merger, though a non-interacting disk feature is also not discluded. There is potential for ongoing star formation present, even though older stellar populations are present, further supported by the tidal tail structure.
