The galaxy presents as a spiral type, with a relatively small bulge and prominent, tightly wound spiral arms. There appears to be at least two to three spiral arms, potentially more, exhibiting a slightly clumpy structure. The disk appears relatively thin and elongated, with a high degree of symmetry. The central bulge region exhibits a slightly yellowish hue. The spiral arms themselves show variations in color, with some patches of blue, suggestive of ongoing star formation, interspersed within a more diffuse, less distinctly colored arm structure. No signs of major disturbances or ongoing mergers are readily apparent. The galaxy exhibits a smooth profile, with the majority of its light concentrated in the central regions.
