The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a high degree of central concentration. A bright, intensely luminous core region dominates the overall morphology. The light gradually decreases in intensity moving outward from the center with no obvious features of disturbance or mergers. There appears to be little to no disk present with the light of the galaxy appearing roughly round. A population of old stars dominate the galaxy, exhibiting a relatively low rate of star formation and a large mass. The galaxy emits a strong, yellowish light due to its aged stellar population.
