The galaxy presents as a relatively smooth, elliptical-like structure with a bright, concentrated central bulge. The color profile suggests a dominant older stellar population, exhibiting a yellowish-red hue in the core region. The outer regions display a slightly bluer tint, potentially indicating some younger stars or ongoing star formation, albeit at a low rate. The galaxy appears largely undisturbed, showing no obvious signs of major mergers or significant tidal interactions. There is a very slight distortion suggesting a potential interaction or a minor disturbance. The shape of the galaxy is moderately elliptical, leaning towards an "in between" roundness but not perfectly spherical. 
