The observed galaxy presents as a spiral galaxy viewed at a moderate inclination. It exhibits a prominent central bulge, surrounded by a disk featuring distinct spiral arms. The bulge appears relatively bright and concentrated. The spiral arms are well-defined, tracing a predominantly two-armed structure, though some arm segments are somewhat fragmented. The winding of the spiral arms appears relatively tight towards the center, transitioning to a more open structure in the outer regions of the disk. Evidence of star formation within the arms is visible through the presence of bluish regions, suggestive of young, hot stars. There is a subtle bar structure bisecting the central bulge. The overall morphology is relatively undisturbed, lacking clear signs of major recent merger events, though some minor disturbances cannot be ruled out.
