The galaxy appears as a relatively smooth, centrally concentrated object with a dominant bulge. The overall color is yellowish-orange, suggesting an older stellar population. There is a hint of a flattened structure, possibly indicative of a disk, though the bulge component is significantly more prominent. Evidence for significant spiral arm structure or star-forming regions is not readily apparent, lending credence to it being a more quiescent system. There is no obvious sign of recent major merger events. The galaxy appears to be somewhat elliptical in shape, with an intermediate axial ratio.
