The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a high degree of luminosity, appearing nearly spherical with a yellow hue, suggesting a high concentration of older stellar populations. Fainter, less concentrated regions extend outwards from the bright core, showing hints of reddish tones that could indicate the presence of dust or a slightly older stellar population compared to the central bulge. There are also subtle hints of bluish color. The overall light distribution is relatively uniform, lacking any pronounced spiral arm structures. The morphology suggests a classification as an elliptical galaxy, potentially in a relatively quiescent state.

