The galaxy presents an elliptical morphology, with a smooth, diffuse light distribution. There is a concentration of light toward the center, suggesting the presence of a bulge. Subtle color variations are visible; bluer hues appear somewhat dispersed in the surrounding regions, perhaps indicative of some star formation activity, although it may be a smaller and subtle amount. Hints of possible disturbances are detected, though the dominant impression is of relative quiescence. No prominent spiral arms or other distinct features are immediately apparent, although the light is slightly asymmetrical in the image.
