The galaxy presents as an edge-on spiral with a prominent, bright central bulge. The bulge exhibits a smoothly distributed luminosity profile. The disk appears relatively thin and elongated, with a noticeable dust lane obscuring the midplane of the galaxy, giving it a somewhat flattened appearance. The color gradient transitions smoothly from the yellowish central bulge to the bluer outer disk. The absence of significant irregularities or tidal features suggests the galaxy has not undergone a major recent merger event, though subtle disturbances cannot be ruled out at this resolution. The overall morphology indicates a relatively quiescent galaxy with ongoing star formation primarily within the disk.
