The galaxy presents a somewhat elongated, elliptical morphology. The central region exhibits a concentrated, bright core. Moving outwards, there is a gradual decrease in luminosity. The color profile shows a redder hue toward the core, shifting to a more greenish tinge in the outer regions. While appearing mostly smooth, subtle undulations suggest the potential presence of underlying disk features or spiral arms, though not clearly defined. No significant disturbances or signs of major mergers are immediately apparent, however the structure might be undergoing a minor interaction. Overall, the galaxy appears relatively undisturbed and possibly in a quiescent state.
