The galaxy presents as an elliptical morphology, exhibiting a smooth and centrally concentrated light distribution. The core region displays a bright yellowish hue, suggesting an older stellar population. A gradual decrease in luminosity is observed from the center outwards. No prominent spiral arms or dust lanes are discernible. A slight distortion is observed in its overall shape, possibly a result of a minor gravitational interaction with another celestial object. The galaxy is a singular object, showing no signs of being in the process of merging with another galaxy.
