The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing more "in between" than perfectly round or elongated. There is a distinct central bulge region that is brighter and more concentrated than the outer regions of the galaxy. The color distribution appears somewhat uniform across the galaxy, with a subtle blueish tint suggesting potential ongoing star formation. There are no obvious signs of strong tidal interactions or major mergers affecting its overall structure. The galaxy seems to have experienced, at most, minor disturbances in its past.
