The galaxy exhibits a largely smooth morphology with minimal discernible internal structure. It appears moderately elliptical, deviating slightly from a perfect circular shape. The central region presents a high surface brightness, suggesting a concentrated nucleus. Color gradients are subtle, with the core exhibiting a slightly bluer hue compared to the redder outer regions, possibly indicating variations in stellar populations or dust content. There is very little evidence of spiral arms or a prominent disk. The light distribution falls off gradually from the center outwards, with no sharp edges or distinct features indicating ongoing major merger activity. Faint extensions or tidal features are not observed.
