The galaxy appears as a centrally concentrated, elliptical-like structure with a smooth light distribution. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. The color profile transitions towards a reddish-orange in the outer regions of the galaxy. There is no clear evidence of spiral arms, dust lanes, or active star formation regions based on visible light analysis. The overall morphology suggests a relatively evolved system. There appear to be no significant tidal disturbances or signs of recent merger events.
