The galaxy presents as a somewhat elongated structure. The central region exhibits a high degree of luminosity, appearing nearly homogenous in color. Faint structures are visible, and may represent spiral arms or tidal tails, however these may be an artifact of image resolution. The color profile is consistent with an older stellar population, given it's red color. The low concentration and size of the galaxy indicate a mass on the order of 10^11 solar masses. The high Sersic index suggest a high degree of central concentration, which is consistent with an elliptical or lenticular morphology. The moderate ellipticity suggests it is not a perfect sphere, and it's position indicates a moderate redshift. Given the red color, and absence of dust lanes, star formation activity is low.
