The galaxy presents a flattened, elliptical morphology. The overall color profile appears to be a gradient, shifting from a bluer hue in its outer regions to a more golden or yellow at the core. This color gradient could be attributed to varying stellar populations and dust distribution, and that this elliptical galaxy is not entirely composed of old stars. The galaxy's major axis is clearly defined, but no distinct spiral arm structures are visible. The light distribution is smooth, with no noticeable clumpy regions of active star formation. The galaxy exhibits a relatively high degree of central concentration, with a bright nucleus that fades gradually into the outer halo. Overall, the galaxy appears to be an evolved system with a mix of intermediate-aged stellar populations, consistent with elliptical classification.