The observed galaxy presents as a spiral galaxy with a moderate redshift, suggesting an intermediate distance. The galaxy exhibits a distinct disk structure with prominent spiral arms, a few of which are clearly visible, demonstrating a classical spiral morphology. The spiral arms appear somewhat tightly wound around the galactic center, suggesting a grand-design spiral structure. The galactic bulge is of moderate size relative to the disk. A bar structure appears to be present, which is of medium strength. There's a suggestion of ongoing or recent interactions or minor disturbances based on slight asymmetries within the spiral arms. The central bulge exhibits a yellowish color indicative of an older stellar population. Patches of blue are observed along the spiral arms, signifying areas of active star formation with younger, hotter stars. The overall luminosity of the galaxy is substantial.
