The galaxy presents as a spiral structure, exhibiting a prominent, moderately sized central bulge. There is some evidence of a bar-like structure spanning about half the width of the bulge along its major axis, with the bar appearing slightly stronger on one side than the other. Two discernible spiral arms emanate from the ends of the bar, which start off tightly wound but gradually become more open. The galaxy displays some evidence of flocculent arms. The galaxy is viewed at roughly a face-on orientation. There are no clear signs of major tidal disturbances or ongoing mergers. The overall color suggests a mix of stellar populations, with the central regions appearing yellower, possibly indicating older stars, while the arms show a hint of blue, suggestive of more recent star formation. The disk is relatively smooth, with a high degree of axial symmetry. The disk shows no signs of being edge-on.
