The galaxy presents a largely smooth, elliptical morphology. A concentration of light toward the central region indicates the presence of a galactic nucleus, which appears slightly redder than the surrounding area. There is a subtle, diffuse halo extending outward from the central core. A slight elongation is discernible in the galaxy's overall shape, deviating from a perfectly circular form. The color profile suggests moderate levels of star formation. No prominent spiral arms or distinct dust lanes are immediately visible, supporting its classification as an elliptical galaxy. There may be some minor gravitational disturbance in the system. 
