The galaxy presents as a spiral type, exhibiting well-defined spiral arms. The arms appear somewhat tightly wound, with a patchy texture indicative of star-forming regions. A central bulge is visible, appearing moderately prominent within the galaxy's overall structure. Dust lanes appear to be interwoven within the spiral arms, creating a complex and mottled appearance. There seems to be a lack of substantial disruption in the main structure of the galaxy, although there is evidence of minor interaction within the spiral arms. The galaxy is tilted with respect to our line of sight, giving us a near face on view.
