The galaxy appears as a centrally concentrated, luminous object. The color is predominantly yellowish-white, suggestive of an older stellar population, particularly in the core. There may be faint blueish-white regions surrounding the bright core that suggest younger stars. There are no obvious spiral arms or a well-defined disk, but subtle variations in light distribution around the central region point to possible weak disk-like features. Some subtle irregular features indicate minor disturbances. The object's radial size is relatively compact. The overall appearance aligns most closely with a galaxy near the elliptical-lenticular boundary, though weak features and irregularities may indicate recent or ongoing interactions. Its estimated mass is significant, though the low star formation rate suggests it is not currently vigorously forming stars.
