The galaxy appears as a centrally concentrated, luminous object. It exhibits a smooth, elliptical morphology, with the highest intensity light emanating from the galactic nucleus. The radial intensity profile suggests a gradual decrease in luminosity from the core outwards. The overall color is redder, implying a relatively older stellar population and lower ongoing star formation activity. There is no obvious spiral arm structure, bar, or signs of recent merger activity visible in the image. The object is moderately round.
