The galaxy presents as a somewhat featureless elliptical, with a high degree of central concentration. It appears relatively smooth, exhibiting a round morphology with a minimal disk component. The color profile indicates an older stellar population, leaning toward redder hues. Possible merger activity or gravitational disturbance may be ongoing, as indicated by some irregularity in the outer isophotes. There may be a faint tidal tail structure to the galaxy. Overall the galaxy is a fairly massive galaxy that has very little active star formation.
