The galaxy appears to be a relatively bright, early-type spiral galaxy, viewed at an oblique angle. It exhibits a smooth, centrally concentrated bulge with a bright nucleus. A flattened disk is present, though the spiral arms are not well-defined, appearing somewhat flocculent and tightly wound. There is a hint of a faint, extended halo surrounding the main body of the galaxy. The overall color is relatively uniform with a slightly yellow hue, which could indicate an older stellar population. There are no obvious signs of active galactic nuclei or a recent major merger event, though there may be some minor morphological disturbances. Overall, the galaxy appears to be in a relatively quiescent state.
