The galaxy presents as a spiral type with a fairly well-defined disk. The spiral arms are prominent and display a clumpy morphology suggestive of ongoing star formation. The arms appear somewhat fragmented, indicative of interactions or internal disturbances. A central bulge is present, exhibiting intermediate size relative to the disk. There may be a weak bar-like structure extending through the galactic center. There is no indication of any major merger event or strong tidal disruption, though minor disturbances cannot be ruled out. Overall, the galaxy presents a classical spiral structure with an active star forming disk at an approximate distance that corresponds to a redshift of approximately 0.24. The galaxy appears to be a fairly massive system, based on its luminosity.
