This galaxy presents as a somewhat disturbed system. The overall morphology suggests a disk galaxy, though the asymmetry is notable. One region, located on the left of the image, shows a distinct orange hue with a concentrated appearance, possibly indicating a significant population of older stars. The other region, on the right, shows a bluer color. There are signs of tidal disruption or interaction. The galaxy's low mass and blue color indicate some level of star formation activity. There is no clear, dominant spiral structure, and no apparent central bulge. Overall, this galaxy exhibits characteristics suggesting it is experiencing some form of external disturbance.
