The galaxy presents an overall smooth appearance, with a slightly elongated morphology suggestive of a possible disk component viewed at an angle. The color gradient transitions from a bluer hue at one edge to a redder hue at the opposite end, possibly indicating differing stellar populations or dust obscuration across the galaxy. There appears to be some irregular structure suggestive of minor disturbances in the galaxy’s overall form, possibly caused by interactions with smaller galaxies or internal processes. The object appears to be actively forming stars at a high rate.
