The galaxy presents as a centrally concentrated, smooth object with an elliptical morphology. There appears to be a high degree of radial symmetry, and a lack of distinct structural features such as spiral arms or a prominent bar. The light distribution suggests a relatively homogenous stellar population. The color appears to be trending toward a slightly redder hue overall, and there is some evidence of blue light concentration in the central region. This suggests the possibility of some ongoing, but low-level, star formation within the core of the galaxy. There does not seem to be any signs of tidal disturbances or interactions with neighboring galaxies, as the outer regions appear fairly undisturbed and regular. The galaxy displays an intermediate level of roundness, neither perfectly spherical nor highly elongated. 
