The galaxy appears as a centrally concentrated object with a smooth morphology. Its overall shape is elliptical, trending towards round, with a high degree of central concentration. The color gradient transitions from a redder core to bluer outer regions, suggesting a decrease in the average age of stellar populations with increasing distance from the galactic center. There is no obvious evidence of spiral arms or a distinct disk component; the galaxy is mostly spheroidal. The apparent smoothness and lack of prominent features suggests that it is unlikely undergoing a major merger, though subtle disturbances may be present. The overall color and morphology hint at a significant population of older stars.
