The galaxy presents as a spiral type, exhibiting prominent and well-defined spiral arms. These arms display a relatively medium winding, suggesting an intermediate stage of spiral arm development. The overall structure indicates a flocculent spiral morphology. The galactic bulge appears moderate in size relative to the disk. The color distribution suggests active star formation regions within the spiral arms, contrasted by a yellower, more evolved stellar population in the central bulge. The galaxy displays no obvious signs of major mergers or significant tidal disturbances, although subtle asymmetries in the outer disk might indicate minor interactions or past accretion events. A weak bar structure is possibly present, but further analysis would be needed to confirm.
