The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The light distribution appears relatively uniform, lacking any distinct spiral arm structures or prominent dust lanes. The overall color gradient suggests a population of older stars, with a redder hue dominating the central region transitioning to slightly bluer tones in the outer regions of the galaxy. There are no apparent signs of significant tidal disturbances or ongoing major mergers, indicating it is likely a relatively relaxed system. Minor disturbances cannot be ruled out. The shape is mostly round.
