The galaxy presents as a somewhat diffuse object, exhibiting a predominantly yellow-orange hue. The morphology appears disrupted, possibly indicative of a merger or tidal interaction. There are irregular clumps of higher intensity emission distributed throughout the central region of the galaxy. There is not a clear, well defined disc structure. The overall visual texture suggests a galaxy with an intermediate redshift, exhibiting both smooth and more feature-rich components, and a significant fraction of ongoing or recent star formation activity. A considerable portion of the galaxy's light emanates from what appears to be older stellar populations, contributing to the orange-red coloration.
