The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that appears yellowish, suggesting an older stellar population with less ongoing star formation. The surrounding halo is more diffuse and appears bluer, possibly indicating the presence of some younger stars. The galaxy is moderately rounded in shape, deviating slightly from a perfect circle. There is no obvious indication of strong tidal disturbances or a major merger event. The overall structure suggests a relatively evolved system, consistent with a large mass and low specific star formation rate. There may be a minor interaction or disturbance, though it is not readily apparent from this image alone.
