The observed galaxy exhibits a clear disk-like structure viewed nearly edge-on. The bulge component appears to be elongated and has a somewhat rounded morphology. The dust lane is prominent and obscures a significant portion of the galaxy's mid-plane. There appears to be evidence of ongoing star formation, particularly in the regions extending away from the central bulge along the disk. It is a relatively large galaxy with some signs of minor disturbances in its structure, although it does not appear to be undergoing a major merger event. The disk shows some bluer regions indicative of active star formation with some areas showing yellower and redder hues indicating the presence of older stellar populations.
