The galaxy presents as a spiral type, exhibiting prominent, loosely wound spiral arms. A central bulge is visible but appears relatively small in proportion to the overall disk size. The arms are traced by regions of enhanced blue luminosity, likely indicating areas of active star formation. A faint bar-like structure is potentially present across the central region, though not definitively strong. The overall color index suggests a mix of older stellar populations and regions of recent star formation. The morphology suggests a relatively undisturbed disk structure, though some minor tidal features cannot be ruled out. There is no apparent dust lane, and no significant ongoing merger activity is apparent in the image.
