The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that appears largely featureless in this image. The galaxy appears more luminous in redder wavelengths, suggesting an older stellar population dominates the light output. There is no evident spiral structure, nor are there strong signs of recent or ongoing merger activity. The object exhibits a fairly circular shape, with a minor asymmetry suggesting only a slight deviation from perfect ellipticity. The size of the galaxy is relatively compact.
