The galaxy exhibits a morphology that appears to be somewhere between smooth and featured, with a hint of disk-like structure. It displays a dominant central bulge with a bright, concentrated core, suggesting a significant concentration of older stars or a possible active galactic nucleus. Fainter emission extending outwards from the central bulge seems to suggest the presence of a disk, although this feature is less defined. There is some visual evidence of possible minor disturbances within the galaxy’s morphology, with indications that tidal features could be present. The galaxy has a redshift of approximately 0.4, putting it at a considerable cosmological distance. This galaxy appears to be fairly massive and actively forming new stars, at a rate that puts it amongst the most productive star forming galaxies in the cosmos. Overall the galaxy appears to be a galaxy that has a mass on the order of 10^11 times the mass of our sun, and a star formation rate roughly less than 10 stars per year.
