The object appears to be a galaxy at an intermediate redshift, exhibiting a degree of interaction or disturbance. The morphology suggests a system that is neither entirely smooth nor a well-defined spiral or elliptical structure. The galaxy displays two main concentrations of light, implying either a close pair of galaxies or a single galaxy with a significant tidal feature or ongoing merger. The primary component is a relatively diffuse and smooth body of light, slightly elongated in shape. A secondary component presents a similar but slightly less luminous and compact appearance. There is evidence of disturbed material between and surrounding the main bodies, evidenced by diffuse blue patches, indicative of star formation triggered by interactions. The overall color suggests a mix of stellar populations, with some regions appearing bluer, and others redder, potentially correlating with different ages of star formation regions within the system.
