The galaxy presents as a somewhat elliptical, disk-like structure. It exhibits a smooth, concentrated central bulge region with a yellow-orange hue, indicating an older stellar population. The outer regions of the galactic disk display a bluer color, suggestive of ongoing star formation. The galaxy appears relatively undisturbed, lacking any significant signs of tidal interactions or major mergers. There might be a slight asymmetry or minor disturbance, but overall, it presents a fairly settled morphology.
