The galaxy presents as a relatively compact, elliptical or lenticular system. It exhibits a smooth, somewhat featureless morphology, suggesting a population of older stars. There is a slight elongation, but the isophotes are generally round. The central region is brighter, indicating a concentration of stars toward the galactic nucleus. The light emitted is skewed toward the redder part of the spectrum, potentially indicative of lower levels of star formation, consistent with an older stellar population. There is some evidence of a very minor disturbance, possibly a very minor merger event. This galaxy is a high mass galaxy, with a relatively low specific star formation rate.
