The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge. The light profile appears centrally peaked, diminishing outwards with no discernible spiral arm structure. The color is generally yellow to orange suggesting an older stellar population and diminished star formation rate. The shape appears mostly round, with only a slight elongation. There is no strong evidence of tidal features or major disturbances indicative of a recent major merger event. Minor asymmetries could suggest minor gravitational interactions or internal processes.
