The target galaxy presents as a single object with a relatively small angular size. It exhibits a complex morphology suggestive of ongoing or recent merger activity. The primary body of the galaxy is diffuse and appears somewhat elongated, but with no discernible spiral structure. There are at least three distinct, high-intensity luminosity peaks within the galaxy. The color profile varies across the galaxy, with a central concentration of yellow, potentially indicative of an older stellar population or dust extinction, with green halos around the yellow. Irregularities in the outer regions indicate a perturbed structure possibly due to tidal interactions. The overall appearance suggests a system undergoing significant dynamical disturbance.
