The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. Its shape appears to be generally elliptical. Color gradients suggest a relatively old stellar population throughout the majority of the galaxy. There are no indications of prominent spiral arms or a well-defined disk structure. Visual inspection suggests there is ongoing star formation, although this appears to be happening at a moderate rate. A small portion of the galaxy shows faint color variations, possibly indicating recent merger activity or minor gravitational disturbance. Overall, the galaxy appears relatively undisturbed and shows minimal signs of major recent interactions.
