The galaxy presents as a somewhat elliptical structure, with a dominant central bulge. This bulge exhibits a yellowish-orange hue, potentially indicative of an older stellar population. There's a subtle flattening observed in the overall shape. The outer regions of the galaxy fade gradually, displaying a bluer tint. This could suggest the presence of younger stars in a disk-like component. The smooth appearance implies a relatively quiescent system. There is a very slight asymmetry in the outer regions, but overall it seems undisturbed. 
