The galaxy presents as a spiral galaxy, viewed at an oblique angle. The central bulge appears relatively small and indistinct, suggesting it might be considered a normal spiral, perhaps of type Sb or Sc.

The spiral arms are prominent but somewhat indistinct, implying moderate star formation activity. The arms appear loosely wound, which suggests the galaxy has not undergone significant recent interactions or disturbances. There are two prominent arms.

There is no evidence of a strong bar structure. 

The galaxy’s color suggests a mix of stellar populations, with a bluer tint, indicating ongoing star formation, most prominent in the disk, and a yellow to red tint in the bulge.

There is no indication of any major merger events. The galaxy appears to be relatively undisturbed, however there may be a minor disturbance indicated by asymmetric features or tidal tails.
