The galaxy presents as an elongated, disk-like structure, viewed nearly edge-on. A prominent central bulge is visible, exhibiting a yellowish-orange hue, suggesting an older stellar population. The disk component appears bluish-white, indicative of younger, hotter stars, and potentially some ongoing star formation. The disk appears relatively smooth with only a slight disturbance, with no obvious signs of strong spiral arm structure or a major merger event. Dust lanes are subtly present and follow the plane of the disk. The overall morphology appears consistent with a relatively massive, late-type spiral galaxy undergoing moderate star formation.
