The galaxy presents a generally smooth, elliptical morphology, with a concentrated central bulge that emits strongly in the yellow-green wavelengths, suggesting an older stellar population. The isophotes appear fairly regular, deviating only slightly from perfect elliptical symmetry. There may be very faint evidence of a disk, although it is almost certainly viewed at a high inclination, nearly face-on. There is no clear evidence of spiral arm structure or other features. It does not appear to be strongly interacting or merging with any other galaxies. Overall, the galaxy appears relatively undisturbed.