The galaxy appears to be a relatively smooth, elliptical galaxy. It has a bright central bulge with a color gradient suggesting a somewhat older stellar population toward the center. The overall shape is quite round, with little evidence of a disk structure or significant tidal disturbances. The faint halo extends for approximately 3 kpc from the center of the galaxy. There is no sign of any recent or ongoing merger activity in the image. The galaxy appears to be a fairly isolated object with a redshift of approximately 0.19, indicating that it is at a considerable distance from us. It has a moderate rate of star formation. 
