The galaxy exhibits a clear spiral structure. Two prominent spiral arms emanate from a central bulge. The bulge appears moderate in size, displaying a yellowish hue, suggesting a population of older stars. The spiral arms themselves are traced by regions of bluer light, indicative of active star formation. These arms show a medium degree of winding. The presence of a bar-like structure is discernible across the central region, adding complexity to the galactic morphology. The galaxy shows no signs of major merging events, though some minor disturbances may be present in the spiral arm structure. There is evidence of dust lanes within the arms, obscuring some of the light from behind.
