The galaxy appears to be an elliptical galaxy, characterized by a smooth and relatively featureless morphology. It exhibits a centrally concentrated luminosity profile, with the brightest region located at the core. The galaxy displays a roughly round shape, showing minimal signs of a disk-like structure. There is no evidence of significant ongoing merger activity or major disturbances within the system. The color gradient suggests an aging stellar population, with redder hues dominating the galaxy's overall color. Star formation appears to be minimal. The galaxy appears to be moderately massive.
