The galaxy presents a somewhat smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile with a gradual falloff towards its periphery. The color indices suggest a population of moderately old stars. The galaxy does not present a strong blue component, suggesting that there is not a lot of on-going star formation. There is no evidence of strong spiral arm structure. The round appearance indicates that it is an early-type galaxy. A hint of a disk structure is present, though not prominent. No evidence of major mergers or strong tidal disturbances are observed, though a minor disturbance can not be ruled out. Overall, the galaxy appears to be a relatively undisturbed, moderately massive system.