The galaxy presents a relatively smooth and concentrated central bulge that transitions into a more diffuse disk. The disk does not appear to be highly structured, lacking prominent spiral arms. The overall color of the galaxy is a pale blue-white, indicating a moderate amount of recent or ongoing star formation within the disk. The shape appears to be somewhat elliptical but approaching circular with a hint of a disk-like structure that is oriented nearly edge-on. There are no obvious signs of a major ongoing merger, though subtle disturbances or interactions cannot be ruled out, with the possibility of a minor tidal disturbance.
