The galaxy presents as a somewhat elongated structure, likely a disk galaxy seen at an angle to our line of sight. There is a prominent central bulge that appears yellow-white in color, suggesting an older stellar population dominating this region. The disk itself is less defined, with a hint of spiral structure visible, although not distinctly resolved. The galaxy appears relatively smooth, indicating the absence of significant ongoing major merging events. There is a minor indication of some disturbance within the disk. The overall color is consistent with a galaxy that may be in the process of ceasing star formation.
