The galaxy presents as a relatively faint, extended object with a disturbed morphology. It appears elongated, with a noticeable asymmetry in its structure. The light distribution is not uniform, showing a brighter, somewhat amorphous central region. Extending from this central area is a diffuse, tail-like feature, suggesting possible tidal interactions or recent mergers. The color appears predominantly blueish, particularly in the extended tail, possibly indicating active star formation regions with populations of young, hot stars. There is no clear evidence of spiral arms or a well-defined disk, but rather a more irregular, perturbed shape. The overall structure implies a system that has undergone, or is currently undergoing, a significant gravitational interaction.
