The galaxy presents a largely smooth morphology, appearing as an elliptical structure. Its overall shape is generally round with a slight deviation towards an intermediate profile. No major or minor disturbances, or tidal tails are apparent, which supports a scenario of minimal recent merger activity. The galaxy appears to be a large, luminous system with a discernible color gradient; its central region presents a redder hue relative to the comparatively bluer outer regions. Given the color profile and smooth morphology, the system is consistent with a high mass and a moderate degree of star formation.
