The galaxy presents as a spiral structure with a relatively compact morphology. The central bulge appears prominent, contributing significantly to the overall luminosity. There are visible arms, though they appear somewhat loosely wound and patchy in their star formation activity. The disk component of the galaxy is evident, but it appears relatively smooth. The color of the galaxy suggests a mixture of stellar populations, with a bluer hue within the arms, potentially indicating ongoing star formation, and a redder color towards the central bulge, indicative of older stellar populations. There is no obvious strong bar structure apparent, nor any prominent features suggesting ongoing major merger activity. The galaxy exhibits a moderate degree of spiral structure. 
