This galaxy presents as a single, relatively smooth, and centrally concentrated object. It appears largely spheroidal in shape, with a hint of elongation. The color gradient suggests an older stellar population, possibly with a concentration of younger, bluer stars in the core region. There is no readily apparent evidence of a disk-like structure or spiral arms. No signs of significant ongoing star formation can be seen. The light distribution is consistent with an elliptical galaxy. There may be very minor indications of tidal disturbances, but on the whole it appears undisturbed.
