The galaxy presents as a somewhat diffuse, irregular structure. Its overall color is primarily bluish, suggesting the presence of a relatively young stellar population and ongoing star formation. There are no clear spiral arms, and the light distribution appears uneven. Some areas look more concentrated, hinting at the presence of denser stellar regions. The galaxy displays evidence of possible tidal disturbances or interactions, as indicated by its asymmetry and the lack of a well-defined, regular morphology. There is a subtle suggestion of multiple nuclei or enhanced star formation, possibly due to a merger event. Overall, the morphology is more consistent with an irregular or disturbed disk galaxy.
