The galaxy presents as a centrally concentrated object with a nearly spherical morphology. It exhibits a bright, prominent core that appears smooth in texture. The galaxy's light profile decreases steadily from the core outwards, with minimal visible structural features, such as spiral arms or a distinct disk. The color gradient suggests a bluer core region, possibly indicating younger stellar populations or ongoing star formation in the central area. The outer regions of the galaxy show a redder hue, which could be indicative of older, redder stars. There appears to be a very slight asymmetry or a minor distortion in the outer regions, hinting at a possible past interaction, though the overall structure is largely undisturbed.
