The galaxy exhibits a moderately luminous profile, with an apparent size consistent with a spiral or irregular type at its estimated redshift. Its morphology suggests a system undergoing some form of interaction, potentially a minor merger event or tidal disturbance. There is a central concentration of light, possibly indicating a bulge, from which fainter arms or streams of material extend. The color gradient implies a range of stellar populations, with some regions exhibiting bluer hues, indicative of younger stars and active star formation, and other regions appearing redder, suggesting older stellar populations. There are also patches of concentrated light along the galaxy which are likely areas with active star formation, and some areas of the galaxy exhibit signs of dust extinction. Overall, the galaxy presents a complex and dynamic structure.
