The galaxy presents as a concentrated, elliptical structure with a smooth, generally featureless appearance. It exhibits a radial color gradient, transitioning from a bright, yellowish core to a dimmer, redder outer region. The overall form is consistently rounded, showing no clear indication of spiral arms or a bar structure. There are no apparent tidal tails or significant morphological disturbances, suggesting a settled, relatively undisturbed system. While the central region is well-defined, the outer regions are more diffuse, indicating a gradual decrease in stellar density. The color profile suggests a likely population of older stars, with a limited ongoing rate of star formation.
