The galaxy presents as a single, relatively smooth object with a centrally concentrated light profile. It exhibits an elliptical morphology, appearing largely spheroidal with a high degree of roundness. The dominant color is a yellow-orange hue, suggesting an older stellar population with fewer young, massive stars and a reduced rate of star formation. There is no obvious spiral structure or prominent dust lanes. Slight distortions are present in one area indicating minor gravitational interactions with another galaxy.
