The galaxy presents a generally smooth morphology, with a high degree of central concentration. It exhibits an elliptical shape, appearing somewhat elongated but largely features a rounded morphology. There is no obvious evidence of spiral arms, a prominent disk structure, or any major merger events. Some minor disturbances or irregularities are not entirely excluded but not clearly present in the data either. The galaxy displays a distinct color gradient, with the central region appearing bluer relative to the outer regions, which tend towards redder colors. The observed color variation indicates likely differences in stellar populations. The galaxy is observed at a redshift indicative of a moderately distant object.
