The object presents as a merging system, with two dominant, luminous cores appearing a yellow-orange hue. These cores suggest concentrated regions of older stellar populations. Tidal features are clearly visible, indicating ongoing gravitational interaction. The galaxy appears disk-like but with disturbances. One possible merger component shows blue-ish hues, suggestive of on-going star formation. The overall light distribution appears relatively concentrated toward the core regions, with fainter, extended emission tracing the merger's tidal features. There appears to be some dust and patchy star formation, but the galaxy looks fairly mature overall.
