The galaxy presents as a spiral type with a prominent disk structure. The spiral arms are loosely wound and well-defined, exhibiting a patchy morphology indicative of active star formation regions. The galaxy appears to have a small to moderate bulge component. Evidence of a weak bar may be present but is not definitive. The overall color suggests a bluer population, indicative of ongoing star formation. There may be signs of minor tidal disturbances or a possible minor merger event, but these are not particularly pronounced. The galaxy is not seen edge-on.
