The galaxy presents as a relatively smooth, elongated structure. It exhibits a prominent central bulge, which appears a yellow-orange hue, suggesting an older stellar population. The disk component shows a greenish tint which can be attributed to ongoing star formation. The galaxy's overall shape suggests a lenticular or possibly an early-type spiral galaxy viewed at a significant inclination. There's no clear evidence of strong spiral arm structure, but hints of disk features are visible. There aren't any obvious signs of major merging events. The edges of the galaxy appear indistinct, fading gradually into the background sky.
