The galaxy presents as a flattened, disk-like structure with a prominent central bulge. The bulge exhibits a yellowish-orange hue, suggesting an older stellar population. The disk appears relatively smooth with a faint blueish tint, hinting at ongoing, but not substantial, star formation. Dust lanes are not clearly resolved, indicating that this galaxy is unlikely to be highly active. Overall, the morphology indicates the galaxy is an early-type spiral galaxy. The elliptical shape suggest the galaxy is angled to our point of view. There are no other visible indicators of recent major interactions.
