This galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an overall elliptical morphology, appearing mostly round, with no discernible spiral arm structures or significant disk component visible. The light distribution suggests a dominant spheroid component. There is a color gradient present, transitioning from a slightly bluer hue in the outer regions to a redder, more centrally concentrated core. The overall color index appears to be redder, suggesting an older stellar population. No apparent signs of ongoing major mergers or significant tidal disturbances are observed in this image.
