The galaxy appears to be a spiral galaxy, observed at an oblique angle. Prominent spiral arms are visible, showing a complex structure. The arms appear somewhat flocculent, with segments of higher luminosity and dust lanes. A central bulge is present but is not particularly prominent. The bulge exhibits a yellowish color, which likely indicates a population of older stars. The spiral arms show a bluer color indicative of ongoing star formation. There is no obvious bar structure present. The overall morphology suggests some possible gravitational disturbances or interactions. There may be evidence of minor tidal features or asymmetry, particularly at the edges of the disk, indicating a past or ongoing minor merger event. Dust is visible throughout the disk of the galaxy.
