The galaxy presents as a relatively smooth, centrally concentrated object. The overall shape is roughly elliptical, appearing more rounded than elongated. A bright central bulge is clearly visible, with the light intensity decreasing gradually towards the outer edges of the galaxy. There is a hint of a faint, extended disk component surrounding the bulge, displaying a slightly bluer hue which might indicate ongoing, albeit modest, star formation. No prominent spiral arms or bar structures are apparent in this image. The galaxy appears relatively undisturbed, showing no signs of major mergers or significant tidal interactions. Overall, it exhibits characteristics consistent with a galaxy having a dominant spheroidal component and modest star formation.
