The galaxy presents as a centrally concentrated object. A smooth, spheroidal structure dominates the overall morphology. A central bulge region is visible, exhibiting a brighter luminosity than the outer regions. The galaxy appears relatively compact, with a radial falloff in surface brightness from the center outwards. Little to no spiral arm structure is discernible, suggesting the galaxy is likely an elliptical or lenticular type. There may be a subtle disk component. The color appears generally consistent with an older stellar population. Star formation is low in the galaxy. Some evidence suggests this galaxy may be undergoing or have undergone a minor merger in the past. The galaxy shows neither a definitively rounded or cigar shape; its shape is somewhat in between.
