This galaxy presents as a generally smooth, elliptical-like object, although it does not seem perfectly circular. The galaxy appears to be relatively undisturbed with no signs of any major merger activity. There may be some slight disturbance, but this is not immediately apparent. A concentration of light, trending towards redder wavelengths, is noticeable towards the galaxy's core. The rest of the galaxy, moving away from the core, shows a distinct trend toward bluer wavelengths. Overall, there appears to be a modest level of star formation occurring within the galaxy, with a potential concentration of older stellar populations near the core.
