The galaxy presents as a disk galaxy with a noticeable central bulge. The bulge exhibits a yellow hue, potentially indicative of an older stellar population, and it dominates the galactic core. The disk appears mottled, hinting at spiral arm structures, though these are not sharply defined. The disk shows a bluer color than the bulge, suggesting ongoing star formation. There is some evidence of minor disturbance in the galaxy's structure. Overall, the galaxy seems to be somewhere between a disk dominated spiral and smooth morphology, likely indicating an intermediate stage in its evolutionary development.
