The galaxy appears to be a spiral galaxy, observed edge-on. It exhibits a prominent central bulge that presents a blue hue. The disk is thin and elongated, with hints of dust lanes or obscuring material visible along the midplane, indicated by the redder regions along the edges of the galaxy. There is no indication of a spiral arm structure, which is expected for an edge-on orientation. The galaxy exhibits a relatively smooth profile, with no significant signs of tidal disturbances or ongoing mergers. The color gradient transitions from a bluer core to redder outer edges of the disk, suggesting a stellar population gradient or dust attenuation. The overall appearance suggests a relatively undisturbed, disk-dominated galaxy.
