This galaxy presents as a barred spiral galaxy, exhibiting prominent, loosely wound spiral arms extending from a central bar structure. The spiral arms are traced by regions of bluer light, suggestive of ongoing star formation activity. The bar appears elongated with a brighter, concentrated central region. The galaxy exhibits an overall flattened disk morphology, with a slight inclination relative to our line of sight. There is evidence of a small bulge component in the central region. The spiral arms show a fairly symmetric distribution, though some asymmetry is noted in the light distribution, perhaps indicating tidal interactions or minor disturbances. The overall color of the galaxy is moderately blue-shifted. There are areas of patchy obscuration within the spiral arms, potentially indicative of dust lanes. The morphology of the galaxy overall suggests a later-type spiral classification.
