The galaxy appears as a centrally concentrated object with a generally smooth morphology. It exhibits an elliptical shape with a high degree of roundness. The color profile suggests a dominant population of older stars, based on the yellowish hue. There are no apparent spiral arm structures or significant dust lanes visible. The galaxy shows no strong evidence of ongoing mergers or major disturbances. The light is fairly uniform, with the brightest region concentrated at the core. There are no indications of recent star formation.
