The galaxy presents a largely smooth, elliptical morphology with minimal discernible features. It appears predominantly round, exhibiting a high degree of radial symmetry in its light distribution. The light profile indicates a centrally concentrated bulge, with luminosity decreasing gradually towards the outer edges. The color suggests a redder stellar population, indicative of an older, more evolved system with a relatively low ongoing star formation rate. There is a slight suggestion of minor asymmetries or distortions in the outer regions, hinting at possible past interactions or minor disturbances, but these are not prominently visible. The galaxy's overall appearance places it within the red sequence, likely a massive galaxy.
