The galaxy presents as a singular, relatively compact object. Its morphology appears generally smooth and elliptical in shape, exhibiting a high degree of roundness. There is some indication of a slight disturbance in its otherwise uniform structure, but no prominent tidal features or signs of an ongoing major merger are discernible. There is evidence of some star formation. The object's color indices indicate a relatively evolved stellar population, though there seems to be some blue contribution, possibly indicative of some ongoing star formation activity. The galaxy is estimated to be roughly 6.6 kpc in radius.
