The observed galaxy presents as a smooth, elliptical morphology, elongated in shape. A dominant central bulge is apparent, exhibiting a concentration of light with a reddish-orange hue. The outer regions show a subtle gradient fading into the background, with hints of a yellowish color, implying a slightly younger stellar population compared to the core. No spiral arms or distinct dust lanes are discernible. The galaxy appears relatively isolated, displaying no signs of major mergers or significant tidal disturbances in its immediate vicinity. The overall structure suggests a well-evolved system, possibly a massive elliptical galaxy with a relatively low ongoing star formation rate.
