The galaxy presents as a relatively smooth, elliptical structure, exhibiting a bright, concentrated central bulge that gradually fades into a less luminous, diffuse halo. The shape is largely rounded, though a slight elongation suggests a deviation from perfect sphericity. There's no obvious evidence of spiral arms or a distinct disk component. The galaxy appears undisturbed, lacking prominent tidal features or signs of ongoing or recent major merger activity. The color gradient indicates an older stellar population, concentrated towards the core, with subtle bluish tinges in the outer regions which might suggest some ongoing low levels of star formation, or a population of younger stars.
