The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a roughly elliptical morphology, appearing quite rounded in shape. A prominent central bulge is observed, displaying a yellowish-orange hue, suggesting an older stellar population dominating this region. Moving outward from the core, the galaxy's color gradually shifts towards a bluer shade, implying the presence of younger, bluer stars in the outer regions, although the overall color is dominated by redder wavelengths. There is no apparent spiral structure or distinct disk. The light distribution appears mostly uniform, with no obvious signs of ongoing major mergers or significant tidal disturbances. It seems to be a massive galaxy. Star formation appears to be low.
