The galaxy presents as a disk galaxy, viewed at an oblique angle. The central bulge appears somewhat indistinct, with a concentrated region of brighter, yellowish light. Extending outwards from this central region are fainter spiral arms, exhibiting a bluer hue suggestive of younger stellar populations. The overall structure displays some irregularity; the spiral arms do not appear entirely symmetrical. There is a hint of tidal distortion or ongoing interaction, possibly a minor disturbance, as evidenced by the asymmetry and the extended, diffuse features at the periphery. Dust lanes are not distinctly visible, though some mottled dark regions within the arms may indicate their presence. There are signs of a significant merger event or major disturbances in the galaxy's morphology.
