The galaxy presents as a spiral type, though the arms are not sharply defined and appear somewhat flocculent. A central bulge dominates the structure, exhibiting a bright, yellowish hue indicative of an older stellar population. Moving outward from the core, the spiral arms display a bluer tint, suggesting more recent star formation activity is present. The galaxy is not perfectly face-on, appearing at a slight incline relative to our line of sight. There's no obvious strong bar structure visible in the central region. The overall shape is not perfectly smooth; there is some subtle clumping and unevenness to the light distribution in the spiral arms, possibly caused by the presence of star-forming regions or dust lanes. There's no obvious sign of major recent mergers or strong tidal distortions. A slight asymmetry is present in the outer disk.
