The galaxy appears to be an elliptical galaxy with a smooth, symmetrical light distribution. The core is a bright, concentrated yellow-white, indicating a population of older stars. There is a subtle, diffuse halo surrounding the core, fading into the background. The galaxy exhibits a slight elongation, but largely maintains a rounded shape. No distinct spiral arm structures or dust lanes are visible, reinforcing its classification as an elliptical galaxy. There is no evidence of any major mergers or disturbances, though there may be a minor distortion to its shape. The overall color suggests it has a lower rate of star formation.
