The galaxy presents as a largely smooth, elliptical-like structure. It appears well-rounded, exhibiting a high degree of symmetry with minimal deviation from a circular form. The light distribution suggests a centrally concentrated luminosity profile, with brightness diminishing gradually outwards. The core is a bright yellow color, fading into a redder hue in the outskirts of the galaxy. There is no readily discernible spiral arm structure, nor is there evidence of significant tidal disturbances or ongoing major merger activity, though very minor disturbances cannot be ruled out. The overall morphology points towards a relatively evolved system, possibly an early-type galaxy with a suppressed star formation rate and substantial stellar mass.
