The galaxy presents as a relatively smooth and concentrated object. It displays a predominantly elliptical morphology, appearing more "in-between" than perfectly round. There is a bright central bulge, suggesting a high stellar density.  The light distribution gradually decreases from the core outwards, with no prominent spiral arm structures or distinct features immediately apparent. The galaxy appears to be largely undisturbed, showing no signs of major mergers or tidal disruptions. There might be hints of minor disturbances within the outer regions of the galaxy. The galaxy displays a color gradient with a bluer core and redder outer regions.
