The galaxy presents a complex morphology, appearing to be in a state of interaction or merger. The central region exhibits a diffuse, disturbed structure with hints of faint spiral arms. There are two bright blue regions within the galaxy suggesting active star formation occurring in those areas. Overall, the galaxy displays a slightly elongated shape, but it's difficult to determine if this is due to an intrinsic cigar shape or a projection effect of the interaction. The lack of a distinct nucleus suggests a galaxy that has undergone significant tidal disruption.
