The galaxy presents a relatively complex structure, appearing to be a spiral galaxy viewed at an oblique angle. The central bulge exhibits a moderate concentration of light, transitioning into a disk structure. Two dominant spiral arms emerge from the central region, exhibiting a moderate winding pattern. These arms are not perfectly symmetrical, suggesting possible gravitational interactions or internal disturbances.

There is evidence of a weak bar structure across the central bulge, possibly contributing to the observed spiral arm morphology. Patches of bluer light are observed along the spiral arms, indicative of active star formation regions. The overall color suggests a mix of stellar populations, with both older, redder stars concentrated in the bulge and younger, bluer stars distributed along the spiral arms.

The galaxy shows evidence of potential ongoing or past interactions. Although there are no obvious merging features, there appears to be some level of disturbance in the disk, where the arms become irregular, and the overall structure is asymmetric.
