The galaxy presents a moderately elliptical morphology, appearing significantly longer than it is wide. It appears as a largely smooth, centralized mass. There is a slight color gradient visible, transitioning from a yellowish-white core region to a more orange hue on the edges. This suggests a possible change in stellar population, the center being composed of hotter, younger stars compared to the edges. There is some subtle asymmetry and possible disturbance in the shape; this may possibly be due to a small, nearby companion galaxy, or some other disturbance.
