The observed galaxy appears to be a relatively luminous, late-type spiral galaxy, seen nearly edge-on. A prominent central bulge is observed, exhibiting a yellowish hue, indicative of an older stellar population. Fainter and bluer light extends away from the bulge along the major axis, suggesting the presence of a galactic disk with ongoing star formation. The galaxy exhibits a moderate degree of smoothness with a slight warp, indicating the possibility of a past interaction or disturbance, but no strong tidal features or obvious signs of an ongoing merger are apparent. The overall morphology suggests a disk-dominated system with a relatively high mass and low star formation rate.
