The galaxy presents as a spiral type, observed at an oblique angle relative to our line of sight. Distinct spiral arms are visible, although somewhat flocculent in appearance. The arms exhibit a bluish hue, suggesting the presence of ongoing star formation. A central bulge is apparent, displaying a moderate size relative to the overall galactic disk. The bulge appears yellowish-white, indicating a population of older stars. The disk component exhibits a general flatness and a lack of pronounced central concentration beyond the bulge. There's no clear evidence of a strong bar structure. No major signs of tidal disturbances or ongoing major mergers are apparent, although minor disturbances may be present. 
