The observed galaxy presents as a spiral type, viewed at an angle substantially offset from edge-on. Its central bulge is relatively small but discernable, exhibiting a moderate concentration of light, grading outward to the galactic disk. Prominent spiral arms are observed, with two dominant arms. These arms exhibit a medium winding, neither tightly wound nor loosely sprawling. No significant distortions or tidal tails are observed, although a minor disturbance or asymmetry within the spiral arm structure cannot be ruled out. Evidence of a bar structure is present.

The bluer color observed throughout the disk suggests ongoing star formation. The core shows up as a bright yellow-white color, indicating an older population of stars.
