The galaxy presents a smooth, elliptical morphology with a high degree of central concentration. Its overall shape is somewhat elongated, resembling a cigar shape. The galaxy's core is bright and yellow, suggesting an older stellar population. The outer regions fade into a more diffuse and slightly bluer halo. No distinct spiral arms or prominent dust lanes are observed, and there is no evidence of any major mergers or significant tidal disturbances. The overall appearance suggests a relatively evolved system with little ongoing star formation.
