The galaxy exhibits a distorted, elongated morphology, appearing cigar-shaped. It shows evidence of tidal disturbances, potentially indicative of an ongoing or recent interaction. The light distribution suggests a complex structure with what could be a disk component and potential tidal tails or bridges. The galaxy displays both smooth and more featured regions, with some areas appearing relatively uniform in color and texture, while others show clumpy, brighter features. The dominant color is a mixture of redder and bluer tones, which could indicate varying stellar populations. The presence of bluer regions may correspond to areas of active star formation while the redder regions indicate older stars. Overall, the object appears to be an active, disturbed galaxy with a moderate amount of star formation.
