The galaxy presents as a relatively smooth, elliptical structure with a prominent central bulge. The light distribution is centrally concentrated, exhibiting a high degree of symmetry. The galaxy's shape is somewhere between round and elongated, appearing only slightly cigar-shaped. There is no obvious presence of spiral arms or a distinct disk component. The color appears to be composed of primarily redder wavelengths indicating an older stellar population with limited ongoing star formation. There is no evidence of any major disturbances to the morphology, such as tidal tails or obvious signs of an ongoing merger. It appears to be an undisturbed, isolated system.
