The galaxy appears to be a relatively smooth, elliptical system. Its central region presents a concentrated, bright luminosity. Moving outward, there's a discernible decrease in surface brightness, transitioning to a more diffuse halo. The morphology suggests a spheroid-dominated structure with minimal indications of spiral arms or significant disk-like components. There is a slight asymmetry or subtle disturbance in the outer regions. The color gradient transitions from yellow-white in the core to a slightly redder hue in the outer regions. The overall form of the galaxy indicates it has a substantial mass. The rate of star formation appears very low.
