The galaxy presents a generally smooth and rounded morphology. There is no apparent disk structure or spiral arms visible at this resolution. The light distribution appears centrally concentrated with a gradual decline in brightness towards the outer regions. There is no strong evidence of tidal features, close companions or major disturbances in its structure, suggesting this is likely an isolated system that is not currently undergoing a major merger event. The color profile is generally uniform, with no obvious signs of distinct stellar populations or recent star formation events occurring in the outer regions. The galaxy has a significant redshift and is likely at a considerable distance. 
