The galaxy presents with a disturbed morphology, potentially indicative of an ongoing or recent interaction. There are multiple luminous clumps, suggesting active regions of star formation or separate galactic nuclei. The overall color is a mix of bluish and reddish hues, which may indicate a diverse stellar population. Some regions exhibit bluer colors, suggestive of younger, hotter stars, while others appear redder, which may point to older populations or dust obscuration. The galaxy appears relatively compact, with no clear spiral arm structure visible.
