The galaxy presents a somewhat elongated, cigar-shaped morphology. It appears relatively smooth in texture, with no immediately discernible spiral arm structures or prominent dust lanes. The color profile suggests a mix of stellar populations, with a somewhat bluer hue towards one end that could indicate areas of more recent star formation. Overall, the object appears to be a relatively low-mass system with a low star formation rate and a redshift suggesting a considerable distance. The lack of significant morphological disturbances or signs of ongoing mergers indicates a relatively quiescent evolutionary state. 
