The galaxy presents with an irregular morphology. The light distribution indicates an object with noticeable disturbances. There are some indications of features, although ill defined, that may indicate a disk-like structure. The galaxy exhibits a dominant blue hue in the central region, suggesting a population of relatively young, hot stars, although it could also be light that is Doppler shifted due to high rates of travel. There is a relatively low concentration of light and a slightly clumpy appearance, indicative of ongoing star formation or recent tidal interactions. Faint redder components are visible throughout the galaxy, these could indicate the presence of a population of older stars. There may be a small merger occurring, or the effects of a recent merger, as evidenced by a tail-like feature at the top and the irregular shape. The image suggests that the galaxy is actively evolving, and the structure is not yet fully relaxed.
