The galaxy presents a generally elliptical morphology, appearing relatively smooth and centrally concentrated. Its overall color is slightly redder, especially toward the core, suggesting an older stellar population dominates the central regions. There is evidence of a subtle, bluer halo surrounding the main body, which could indicate the presence of younger stars or ongoing star formation, although the rate appears low. The galaxy exhibits a slight deviation from perfect circularity, indicating a possible flattened structure. There are no obvious spiral arms, bars, or other features indicative of a spiral galaxy. The galaxy appears relatively undisturbed with no signs of major tidal interactions or recent mergers.
