The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth, spheroid morphology. There is a slight elongation visible, although it appears mostly round. A prominent central bulge dominates the structure, with a gradual decrease in surface brightness outwards. There is a faint suggestion of a disk component.

The color is generally yellowish-orange. This indicates an older stellar population, with a relative lack of active star formation. The galaxy appears to be relatively isolated with no signs of any major interactions or mergers. There may be evidence of minor disturbances.
