The galaxy presents as a face-on spiral, exhibiting a prominent disk structure with well-defined spiral arms. These arms appear somewhat flocculent. The galaxy's central bulge is moderately sized and displays a yellowish hue, indicative of an older stellar population. There may be a weak bar. The spiral arms show hints of bluer regions, suggesting ongoing star formation within these areas. The overall light distribution suggests a moderate concentration towards the center. There is no obvious sign of a major merger, although the slight asymmetry in the spiral arm structure could potentially indicate a minor interaction or disturbance.
