The galaxy presents as an elliptical or lenticular galaxy with a generally smooth morphology. The light is concentrated toward the center, as expected. The major axis appears to be a few times larger than the minor axis, suggesting a moderate ellipticity. There is a color gradient within the galaxy, with the central region appearing more yellow-red and the outer regions having a bluer hue. While the overall structure is smooth, subtle irregularities in the outer regions may indicate a very minor interaction or disturbance. The high degree of smoothness in the galaxy implies a relatively old stellar population.
