The galaxy presents as a barred spiral type, viewed at a relatively face-on orientation. A distinct bar structure is visible, extending through the galactic center. Spiral arms emanate from the ends of this bar, displaying a relatively tight winding pattern. These arms are traced by regions of star formation, indicated by their bluer color. The central bulge appears moderately sized and exhibits a yellower hue, suggesting an older stellar population compared to the arms. No major disturbances are visible, though some slight asymmetry in the spiral arm structure may indicate a past minor interaction. The overall morphology suggests a well-formed and relatively undisturbed spiral galaxy.
