The galaxy presents as a spiral type, exhibiting a discernible disk structure. The spiral arms are prominent, displaying a relatively open morphology. There is evidence of ongoing star formation activity within the arms, indicated by the presence of bluer regions that likely correspond to populations of young, hot stars. A relatively small or non-existent bulge is observed in the center. The overall color suggests a mix of stellar populations, with a contribution from both older, redder stars and younger, bluer stars. The disk is not perfectly face-on, presenting a slight inclination to our line of sight. There appears to be a minor disturbance in the galaxy's morphology suggesting a possible interaction or past merger event. 
