The galaxy presents as a centrally concentrated object with a generally smooth morphology. Its light profile appears relatively symmetrical. The core exhibits a yellowish-white hue. The galaxy has a notably round shape with hints of a more diffuse, fainter halo extending beyond the central region. The galaxy does not show any obvious spiral arm structures or significant irregular features, suggesting it could be an elliptical or lenticular type, although the resolution limits a definitive classification. There are no indications of a major ongoing merger or tidal disruption. The color indices suggests a population dominated by older stars with moderate active star formation in a lower range. The estimated mass is consistent with that of a typical massive galaxy.
