The galaxy appears as a relatively smooth, elliptical structure. The central region exhibits a higher concentration of light, suggesting a prominent galactic nucleus or bulge. The light gradually fades as it extends outward. There is a slight bluer tinge in the outermost regions of the disk. There appears to be some distortion in the structure of the galaxy. The galaxy is probably a member of the green valley group of galaxies. It appears to be an intermediate mass galaxy with a moderate amount of star formation occuring.