This galaxy exhibits a moderately perturbed morphology, potentially indicative of ongoing or recent interactions. It presents a primarily bluish hue, suggesting active star formation, concentrated predominantly toward one side of the structure. A noticeable reddish component is located centrally, likely indicating an older stellar population and potentially a more concentrated region of dust. The overall form appears somewhat amorphous, lacking the clear spiral arm structure of grand design spirals or the elliptical shape of more evolved galaxies. There is an overall irregular appearance to the distribution of light within the galaxy. This is probably a disk galaxy that is in the process of merging.
