The galaxy presents as a spiral type, viewed at an angle between face-on and edge-on. A prominent, moderately sized bulge is visible. Faint spiral arms are present, though not sharply defined. The disk appears relatively smooth, suggesting ongoing star formation, with no major disturbances. The galaxy does not exhibit evidence of a strong bar structure, with a weaker bar being possible. There is no visually apparent ongoing merging activity with other galaxies, though there are minor disturbances in the disc that cannot be immediately identified.
