This galaxy appears to be a spiral galaxy, oriented at a significant angle relative to our line of sight. It exhibits two prominent spiral arms emanating from the central bulge region. The arms appear somewhat tightly wound, with a moderate concentration of star formation occurring along the spiral arm structure. 

The central bulge is prominent and moderately sized in relation to the disk. There is no obvious bar structure visible across the bulge region. The spiral arms extend smoothly from the center of the galaxy, with no obvious signs of major disturbances, though there may be a minor asymmetry in one of the arms. The overall structure indicates it is not currently undergoing a major merger. The galaxy has a central core with some active star formation, surrounded by a cooler, less active disk of older stars.
