The galaxy presents a generally elliptical morphology, appearing relatively smooth and concentrated. A prominent central bulge is evident, displaying a bright, nearly uniform luminosity profile. The color of the bulge appears slightly redder compared to the outer regions, suggesting an older stellar population. 

Surrounding the bulge is a fainter, more diffuse halo. This halo extends further along the major axis of the galaxy. The halo appears to be relatively smooth, with no distinct spiral arm structure or prominent dust lanes visible. There may be a slight asymmetry or minor perturbation in the outer regions, hinting at a possible past interaction or merger event, but this is subtle. The overall light distribution indicates a relatively evolved system, likely an elliptical or lenticular galaxy.
