The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology is generally ellipsoidal but with some irregularity. There is a suggestion of a disk. The primary body of the galaxy exhibits a blue hue, indicating the presence of younger stellar populations. Near one edge is a distinct reddish area.

The overall light distribution suggests a relatively low star formation rate, but that some recent star formation activity is likely present in at least one region. There is no obvious evidence of a major merger or strong tidal disturbance, but possibly some disturbance.
