The galaxy presents a generally smooth and concentrated morphology. The light distribution is centrally peaked, with a gradual decline in intensity towards the outer regions. The overall shape appears roughly elliptical, tending towards circular, with no discernible spiral arm structures or significant disk component visible. The color profile indicates a dominant yellowish hue in the central region, possibly indicative of an older stellar population, with hints of bluer colors towards the edges. There are no obvious signs of major ongoing mergers or tidal disturbances. The overall appearance suggests a galaxy that has largely completed its major phase of evolution.
