The galaxy appears as a singular, centrally concentrated object with a generally smooth morphology. The light profile suggests a centrally dominant bulge. The galaxy exhibits a somewhat spherical shape. There is a very slight disturbance in the upper left quadrant. Color gradients suggest it is redder in the center and slightly bluer toward the outer regions, perhaps indicating older stellar populations are concentrated in the central bulge. There is no clear evidence of spiral arm structure or a prominent disk. The galaxy is likely an elliptical galaxy, or possibly a lenticular galaxy viewed nearly face-on.
