The galaxy presents as an elliptical or lenticular structure, exhibiting a generally smooth morphology with some features. It has an apparent size of approximately 2.8 kpc in radius based on estimated half light radius, and possesses a predominantly rounded form, though it is somewhat elongated. Colors suggest a degree of aging stellar population, with more light emitted in the redder bands than bluer bands. There seems to be ongoing, although relatively low, levels of star formation occurring within certain regions. There is no signs of any major merger activity.
