The galaxy exhibits a primarily smooth morphology with a discernible central bulge that appears nearly spherical. The light distribution suggests a relatively high degree of central concentration. There is a faint, diffuse halo surrounding the core region, extending outwards. The overall shape approximates a circular profile, but there is a slight elongation that might suggest a transition between elliptical and lenticular classification. There is a subtle suggestion of a possible minor disturbance in the outer regions, without obvious signs of major merger activity. The color profile of the galaxy suggests an aging stellar population, exhibiting a redder hue, although some bluer regions are discernible. The surface brightness appears relatively uniform across the main body of the galaxy.
