The galaxy appears to be undergoing a significant merger or interaction event. There are two distinct, bright concentrations of light suggesting the presence of at least two galactic nuclei. These cores exhibit a reddish hue. The overall morphology of the system is disturbed, lacking a clear spiral or elliptical shape, with tidal features or extended diffuse light indicative of gravitational interaction between the merging components. There seems to be a concentration of older stars, based on the color. The system's estimated size suggests it's a sizable structure at its redshift. Star formation may be ongoing, but at a relatively low rate.
