The object appears to be a galaxy undergoing a significant interaction or possible merger. The primary component presents as a disk-like structure with a noticeable dust lane bisecting it horizontally. This lane is distinctly redder in color, suggestive of dust obscuring background light. The overall color of this disk is a muted yellow-green.

Below the main disk is a somewhat distinct, less structured, roughly spherical component exhibiting a more yellow hue. This may represent a second galactic nucleus, indicating an ongoing merger. The edges of this galaxy system seem disturbed, which could be signs of tidal forces. This distortion lends credence to the merger hypothesis. Further analysis is needed to ascertain the redshift and precise nature of the interaction.
