The galaxy presents a smooth, rounded morphology. The light distribution is concentrated towards the center, suggesting a high degree of central mass concentration. There is no distinct disk component or spiral arm structure visible; instead, the galaxy appears spheroidal. The color gradient appears relatively uniform across the galaxy, implying a homogeneous stellar population. The overall color suggests that this is an older galaxy with a low star formation rate. There is no obvious sign of any interaction with a neighboring galaxy. The redshift indicates that it is located at a considerable distance.
