The galaxy presents a largely smooth morphology, with a high degree of central concentration. Its overall shape is nearly circular, exhibiting minimal elongation. There are no apparent spiral arm structures or significant asymmetries within the visible light distribution. A slight hint of possible disruption is located in the galaxy. It is observed at a redshift indicating that the galaxy is receding from us at a substantial fraction of the speed of light. The galaxy's color suggests the presence of both young and old stellar populations contributing to the overall light. There is also a lack of blue color, indicating there isn't much recent star formation.
