The galaxy appears to be a relatively smooth, elliptical galaxy. The light is concentrated towards the center, indicative of an older stellar population, with yellow and reddish hues dominating the color profile. There is little evidence of a disk structure or spiral arms; the light distribution is generally uniform and decreases gradually with distance from the center, as if it had a higher sersic index. It seems to be relatively undisturbed, with no obvious signs of tidal tails or mergers.
