The galaxy presents a generally smooth, elliptical morphology. The galaxy exhibits a concentrated central bulge region that is approximately circular in shape. Moving outwards from the center, the galaxy's light gradually fades into a more diffuse halo. The color profile indicates a predominantly older stellar population, as evidenced by the yellowish-orange hue concentrated in the central bulge. The outer regions show hints of bluer colors, indicating some presence of younger stars, but the overall star formation rate appears relatively low. The overall shape suggests a relatively relaxed system with no major distortions or ongoing merger events readily apparent. There might be some very minor disturbances or features, but they do not significantly disrupt the overall smooth morphology of the galaxy.
