The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The color profile suggests a higher concentration of older stellar populations, particularly in the core, exhibiting a yellowish-red hue. The light appears to fade gradually from the central region outwards. There is a slight elongation in its shape. There is no clear evidence of spiral arm structure, dust lanes, or active star formation regions visible in this image, supporting the hypothesis that the light is dominated by older stars. There is no apparent distortion indicative of a major merger event. Faint bluer areas, possibly younger stars, appear away from the core, indicating a recent period of low star formation.
