The galaxy exhibits a spiral morphology, presenting with a clearly defined disk structure. This disk shows a moderate inclination relative to our line of sight. The spiral arms are prominent and tightly wound. A strong bar feature is evident, extending through the central region of the galaxy. The bulge is moderate in size, neither dominating nor insignificant relative to the overall galactic structure. The galaxy's light profile suggests a smooth distribution, with little evidence of major mergers or significant disturbances. Colors appear bluer in the outer disk, indicative of recent star formation.
