The galaxy appears as a relatively compact object. Its morphology seems to be somewhere between smooth and featuring a disk component. There are hints of some disturbance or feature in the morphology, possibly an early stage interaction or minor merger evidenced by slight asymmetries in the light distribution. The main body of the galaxy exhibits a somewhat spheroidal shape with a concentration of light in the center, suggesting a substantial bulge component. The color of the central region is a bit redder than the outer parts, which are slightly bluer. This could indicate older stellar populations in the central bulge, and ongoing or recent star formation in a weak disk component.
