The galaxy appears to be a spiral galaxy with a disk-like structure, exhibiting a smooth, elongated morphology. Its overall color index suggests a mix of stellar populations, but with a slight dominance of older stars, particularly towards the central bulge. The galaxy has moderate luminosity. There is a subtle indication of dust lanes or spiral arm structure but this is difficult to ascertain due to the scale of the image. The galaxy does not show strong evidence of recent major merger events.