The galaxy presents as a slightly elongated, diffuse object with a smooth overall appearance. Its color profile is primarily a warm yellow hue, suggesting a population of older stars. There is no discernible spiral structure or distinct dust lanes evident in the image. The object is centrally concentrated, with a gradual fading of light intensity toward its outer edges. Minimal disturbances are visible, indicating a stable, non-interacting system. The overall morphology suggests a likely elliptical galaxy or a lenticular galaxy viewed at a shallow inclination. The galaxy exhibits low star formation activity based on the lack of blue light. Its moderate size and luminosity imply a substantial stellar mass.
