The object appears to be a spiral galaxy, viewed nearly edge-on from our perspective. It exhibits a prominent, elongated bulge, likely populated by older stars, giving it a reddish-orange hue. The disk is visible as a flattened structure extending outwards from the bulge. The galaxy shows a relatively smooth, undisturbed morphology, suggesting a lack of recent major merger events. There is a hint of blueish light in one area outside the center of the galaxy, possibly indicating regions of active star formation within the disk.
