The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge with a high degree of circularity. The light distribution appears largely uniform and symmetric, suggesting a lack of significant spiral arm structures. The color gradient transitions from a yellowish-white core to a slightly redder halo, indicating an older stellar population and potentially less active star formation. There may be subtle evidence of a minor interaction or disturbance, as hinted by a slight asymmetry or faint tidal feature but it does not show any signs of major recent merging activity. Overall, the galaxy appears morphologically evolved.
