The galaxy presents a complex morphology, appearing as a system undergoing a significant interaction. The overall shape is irregular, with a disturbed and asymmetrical structure. There appear to be two main luminous concentrations within the galaxy, suggestive of either two distinct nuclei or a single nucleus with a prominent tidal feature. The light distribution is diffuse, indicating widespread star formation or a significant population of older stars.

There are hints of faint, extended tidal tails or bridges emanating from the central regions, further supporting the conclusion of an ongoing or recent merger event. There are no clear spiral arm structures evident; rather, the overall appearance is chaotic. A modest bulge may be present, although difficult to precisely characterize due to the disruptive interaction. Dust lanes or patches are not readily apparent within the galaxy, however, these details may be obscured by the limited resolution of the image. The system lacks a clearly defined disk component, which is consistent with a merging system that may have disrupted its original disk structure.
