This galaxy presents as a spiral type, exhibiting a prominent disk structure. The spiral arms are tightly wound and somewhat fragmented, displaying a flocculent morphology with distinct regions of star formation evident as subtle blue knots within the arms. The central bulge appears relatively small and moderately bright, gradually fading into the surrounding disk. The overall color profile suggests a mix of stellar populations, with a slightly redder core indicative of older stars and bluer spiral arms suggesting active star formation regions. There is potential evidence of a weak bar structure bisecting the central region. No major tidal features or signs of ongoing mergers are distinctly observable, although some irregularities in the disk suggest minor gravitational disturbances may be present. The galaxy’s orientation is close to face-on, providing a clear view of its spiral structure.
