The galaxy presents a somewhat amorphous morphology with no clear spiral arm structure visible in this image. It appears to be undergoing a possible interaction or merger, with some disturbances in its overall shape. There are indications of some clumpy regions of higher concentration, possibly areas of active star formation, although it is unclear from this image alone. The galaxy exhibits a color gradient with some reddish hues, particularly in some of the core regions, suggesting a potentially older stellar population in these areas. The outer regions are fainter and more difficult to discern. The light distribution is not perfectly smooth; there is some evidence of substructure and disruption.
