The galaxy presents as a primarily smooth, elliptical object. The central bulge is distinctly bright, exhibiting a yellowish hue, indicative of an older stellar population. The outer regions of the galaxy show a gradual fading in luminosity, with a more reddish tint, likely due to cooler, older stars and dust absorption. The galaxy appears generally rounded in shape. There is no obvious indication of strong tidal disturbances or ongoing major mergers. It is likely a massive galaxy with a suppressed star formation rate, as the overall color indicates an older, quiescent stellar population.
