The galaxy presents as a generally smooth, elliptical-like structure with a bright, concentrated central region. The core exhibits a yellowish hue, transitioning outward to a more diffuse, greenish-blue halo. The overall shape is largely rounded with some irregularity. There is no obvious spiral arm structure or evidence of a distinct disk. The galaxy appears relatively undisturbed, showing no major signs of ongoing merger activity or significant tidal disruptions. Its morphology suggests an evolved stellar population with minimal active star formation.
