The galaxy presents as a smooth, elliptical-like structure with a concentrated central bulge. The core exhibits a yellowish-orange hue, suggesting an older stellar population. The overall color gradient transitions to a slightly bluer tint towards the outer regions, hinting at the presence of younger stars, although this is not distinctly pronounced. There is some faint disturbance noted in the galaxy, but the galaxy is not undergoing a major merging event. 
