The galaxy presents a spiral morphology, appearing relatively face-on from our vantage point. Its overall structure is dominated by a central bulge region that exhibits a yellowish hue, suggesting a population of older stars. Faint spiral arms extend outwards from the bulge. The arms appear somewhat flocculent and loosely wound. The bluish tint in the outer regions indicates the presence of younger, hotter stars and ongoing star formation, though not intensely so. There may be some minor tidal disturbances. The shape is somewhat rounded, and does not show any cigar shaped morphology.
