This galaxy appears to be a disk galaxy, potentially with a significant bulge. The bulge region exhibits a bright, concentrated core, suggesting a high stellar density. The disk component shows evidence of some structure, although it is somewhat smoothed or flocculent. Blue colors present in the disk likely denote the presence of younger, hotter stars and active star formation. 

There appears to be some distortion or minor disturbance in the outer regions of the disk, potentially indicating a past or ongoing interaction with another galaxy, or internal dynamics. The overall color gradient suggests a radial decrease in star formation activity from the center outwards. The galaxy is of intermediate size and luminosity for this redshift.
