The galaxy appears to be an elliptical or lenticular galaxy, displaying a relatively smooth and featureless morphology. The light distribution indicates a high degree of central concentration, with a bright, yellowish core transitioning outwards to a fainter, greenish-yellow halo. The overall shape is more oblate than spherical, displaying a moderate degree of ellipticity. There are no immediately apparent signs of spiral arms, bars, or major disturbances indicative of recent mergers or interactions, although subtle irregularities cannot be ruled out at this resolution. The colour gradient suggests a possible radial variation in stellar populations, with the core potentially dominated by older, redder stars, and the outer regions possibly exhibiting a bluer population.
