The observed galaxy exhibits a clear disk structure, presented at a slight angle relative to our line of sight, but not precisely edge-on. Distinct spiral arm features are evident. The arms appear somewhat flocculent, displaying a mix of concentrated star formation regions and diffuse stellar distribution.

The central bulge is subtle, appearing small relative to the overall disk size. A bar feature appears to be present, possibly moderate in strength, extending through the central region.

There are signs of disturbance throughout the galaxy, indicating a merging process that is either an ongoing merging process or a relatively recent past event. These disturbances take the form of asymmetry in the spiral arm structure. The overall color suggests the presence of a wide range of stellar populations, with bluer regions corresponding to ongoing star formation.
