The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. It exhibits a yellowish-white hue, suggesting a stellar population that is dominated by older, evolved stars. There is little evidence of spiral arm structure or dust lanes, further supporting its classification as an elliptical galaxy. The galaxy appears relatively undisturbed, with no signs of major mergers or tidal interactions with neighboring galaxies. It does not seem to be perfectly circular, presenting a slightly elongated shape. There is a subtle color gradient across the galaxy, with the central region appearing more yellow and the outer regions trending towards a slightly redder tone. This may indicate variations in stellar populations or metallicity across the galaxy.
