The observed galaxy appears as a disk galaxy, seen edge-on relative to our line of sight. A prominent central bulge dominates the galaxy's core, with a mostly round, classical morphology. The disk component extends laterally from the bulge, appearing relatively thin. The galaxy exhibits a yellow-orange hue, indicative of an older stellar population. There appears to be a lack of defined spiral structure within the disk, and a general smoothness suggests ongoing or recent star formation activity. The absence of strong dust lanes or significant irregularities implies a relatively settled dynamic state, despite some minor disturbances that may exist in the galactic arms. Overall, the galaxy presents an organized structure with a well-defined bulge and a smooth, although still slightly disturbed, disk.
