This galaxy presents a predominantly smooth and rounded morphology. There is a central bright region, appearing almost spherical in shape, that dominates the visible light output. The light is relatively concentrated and appears to have a relatively high surface brightness. Based on its redshift, this galaxy exists at a considerable distance. There is a subtle colour gradient visible, with the core exhibiting a bluer hue transitioning to a slightly redder and fainter periphery. This colour variation may indicate differences in stellar populations and/or dust content across the galactic structure. No obvious spiral arms or distinct features are discernible, suggesting a relatively featureless profile. There may be some minor disturbances in the outer areas.
