The galaxy presents a generally smooth morphology, with a high degree of central concentration of light. The overall shape appears largely elliptical, tending towards round. There is a possible hint of a disk, but is faint. There is no obvious bar structure. The color profile suggests a relatively homogenous stellar population, with a slight indication of redder hues in the outer regions. No strong tidal features or signs of recent major merger activity are apparent, suggesting a relatively undisturbed evolutionary history.
