The galaxy presents as a spiral type, exhibiting a prominent disk structure. The arms are well-defined but tightly wound around the central bulge. The bulge appears moderately sized relative to the disk. There is a suggestion of flocculent spiral arms, indicating ongoing star formation within the galaxy. There is also a suggestion of a bar structure in the center of the bulge. The disk itself is viewed at a slight inclination. No significant signs of major mergers or tidal disturbances are observed, although minor disturbances may be present.
