The galaxy presents as a disturbed spiral structure, exhibiting evidence of tidal interactions and potential merging activity with a nearby companion. Definite spiral arms are observed, showing a relatively flocculent morphology rather than grand design structure. The arms appear somewhat disrupted, which suggests gravitational interactions, especially between this galaxy and its observed companion. There is a noticeable asymmetry in the disk, further supporting the influence of external forces. The system has a relatively low redshift. Overall, it exhibits characteristics consistent with a star-forming system.
