This galaxy appears to be a relatively smooth, single-component system. There are no obvious spiral arms or a central bar structure visible. Its morphology is broadly elliptical or lenticular, with a somewhat rounded shape. While no major disturbances are seen, there are signs of minor disturbances. The light profile is generally smooth, suggesting a well-mixed stellar population and no significant dust lanes or patches. The color indices suggest intermediate star formation activity. The size suggests it is a galaxy of substantial mass and luminosity.
