The galaxy presents as a spiral type, exhibiting prominent spiral arm structures. These arms appear relatively tightly wound around a central bulge. The bulge itself seems to be of moderate size.

The galaxy's disk is viewed at a relatively face-on orientation. Evidence of a bar structure is subtle, but cannot be ruled out. The morphology does not suggest any major ongoing merging events, although subtle disturbances are present.

The overall color suggests a mix of stellar populations, likely with both older, redder stars concentrated towards the bulge and younger, bluer stars within the spiral arms.
