The galaxy appears to be a relatively smooth, elliptical type galaxy. The central region exhibits a brighter, more concentrated luminosity, suggestive of an older stellar population. The outer regions appear more diffuse. Overall, the galaxy shows a general intermediate elliptical shape, not perfectly spherical but not highly elongated either. There is a hint of minor disturbance on one side of the galaxy, possibly related to a gravitational interaction or accretion event in its past. There is a patch of some sort of active star formation somewhere within the galaxy.
