The galaxy presents a smooth, elliptical morphology. There is a noticeable central bulge which transitions smoothly into the outer regions of the galaxy. The galaxy exhibits a color gradient, with the central region appearing more yellowish, suggesting an older stellar population dominating this area. The outer regions show bluer hues, which could indicate the presence of younger stars. There are no obvious signs of spiral arms or a distinct disk structure. The galaxy appears largely undisturbed, lacking any prominent tidal features or signs of ongoing major mergers. It is likely a mature system, with a substantial stellar mass and moderate star formation activity. The overall shape is somewhere between round and elongated. There is a slight possibility of some minor interaction or disturbance occurring, as there is some asymmetry in the outer halo.
