The galaxy presents as a centrally concentrated, elliptical-like system. The light profile appears smooth, lacking any prominent spiral arm structures or distinct features, suggesting a relatively evolved morphology. The color gradient indicates a population of older stars dominating the central region, transitioning toward slightly bluer colors in the outer regions, hinting at possible ongoing, but subdued, star formation. There is no apparent dust lane or any strong evidence of recent or ongoing mergers, though a very slight asymmetry cannot be entirely ruled out. The galaxy exhibits an overall regular shape, appearing neither highly elongated nor strongly disturbed.
