The galaxy presents as a spiral type, with discernible arm structures. The arms appear relatively tightly wound, suggesting a classification towards the Sa or Sb end of the Hubble sequence. The disk of the galaxy is not perfectly face-on, exhibiting a slight inclination with respect to our line of sight.

There is a prominent central bulge, with the majority of the light concentrated in the bulge region. The colour of the bulge is distinctly yellower/redder than the arms, indicative of an older stellar population. 

Spiral arms display bluer hues, suggestive of ongoing star formation activity. Some patchiness is observed within the arms, potentially indicating HII regions or dust lanes.

Overall, the galaxy exhibits a structure consistent with a spiral morphology, with a dominant bulge component, and evidence of star formation in the spiral arms.

There also seems to be merging activity occuring. 
