The galaxy displays a distinct spiral structure. Two prominent spiral arms emanate from a moderately sized central bulge. The arms appear tightly wound and relatively well-defined, tracing a clear path around the galactic core. The color distribution suggests active star formation within the spiral arms, indicated by the bluish hues, while the central bulge exhibits a yellower, potentially older stellar population. The overall morphology is dominated by the disk component, with evidence suggesting the presence of a bar structure across the central region. There are possible signs of minor tidal disturbances. Overall, this galaxy appears to be a well-formed spiral system with ongoing star formation activity.
