The galaxy presents as a spiral type, exhibiting a disk-like structure. Multiple spiral arms are discernible, tightly wound around the galactic center. The central bulge appears relatively small, with a moderate luminosity gradient transitioning to the disk. The overall morphology suggests no significant ongoing merger events, though subtle disturbances within the spiral arms may indicate minor gravitational interactions. The color profile indicates a mix of stellar populations, with a yellower central bulge potentially populated by older stars, and bluer spiral arms indicative of more recent star formation. The galaxy is observed face-on, providing a clear view of its spiral structure. There is a possibility that this galaxy is barred but it is difficult to tell.
