The galaxy presents as a spiral, observed at a near face-on orientation. Distinct spiral arm structures are evident, displaying a somewhat grand design. The arms exhibit a bluer color, suggestive of active star formation regions populated with younger, hotter stars. There appears to be a moderate central bulge, with a yellowish hue potentially indicating an older stellar population. The disk of the galaxy is relatively prominent, exhibiting a heterogeneous mix of light concentrations and less dense regions. There is no substantial evidence of ongoing major merger activity, though there are some subtle asymmetries that may indicate minor tidal interactions or disturbances. Overall, the galaxy appears to be a well-defined spiral with a significant rate of star formation within its arms. The color variation between the bulge and disk suggests differential stellar populations and evolutionary stages. The galaxy does not seem to be especially smooth and does seem to have a disk. There is a sign of a bar.