The galaxy presents as a spiral type, exhibiting a well-defined disk structure. Two prominent spiral arms emanate from the central region, displaying a grand design morphology. The arms appear to be loosely wound, extending outwards from the core. A central bulge is visible but appears subdued in size relative to the overall disk. The presence of a bar is subtly indicated through a slight elongation and increased density of stars running through the galaxy's central region. The disk is presented at an intermediate inclination. There is no obvious evidence of any ongoing major mergers, but potentially there are minor disturbances. Based on its color and arm structure, star formation activity appears to be moderate throughout the disk, primarily within the spiral arms.
