The galaxy presents a distinct spiral morphology, characterized by tightly wound spiral arms emanating from a central bulge. The bulge appears moderately prominent and exhibits a yellowish hue, suggesting a population of older stars. The spiral arms display a bluish tint, indicative of ongoing star formation. The galaxy appears relatively isolated, showing no obvious signs of major tidal disturbances or interactions with other galaxies, though there appears to be a very slight minor disturbance. The spiral structure consists of two main arms. A strong bar structure appears to be present. The galaxy is viewed close to face-on. 
