The galaxy presents as an elliptical morphology, appearing largely smooth and relatively undisturbed. It exhibits a concentrated central bulge that is surrounded by a more diffuse halo. The color appears to be skewed slightly red, suggesting a population of older stars. There is a slight elongation in its shape, tending towards a somewhat flattened spheroidal form rather than a perfect sphere, but it is in between round and cigar-shaped. There is little evidence of spiral arms or active star formation in this image, with no visible dust lanes. Its structure suggests that it is not undergoing a major merger or significant tidal interaction with any nearby galaxies. There are no indications of strong tidal tails or other merger remnants.
