The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a centrally concentrated bulge, with a gradual decrease in luminosity extending outwards. The color profile suggests a slightly redder hue, indicative of an older stellar population and a relative lack of ongoing star formation. There is no apparent disk structure or spiral arm morphology. The shape is more intermediate than perfectly round, appearing slightly elongated. There's no visual evidence of major mergers or significant tidal disturbances affecting the galaxy's structure.
