The observed galaxy exhibits a complex morphology, with an apparent central bulge structure. This bulge shows a slightly elongated shape. A disk-like structure appears to be present, however it is not well-defined and exhibits some irregularity. One side of the galaxy shows what appears to be a tidal tail emanating outward from the central region. The color distribution across the galaxy indicates variations in stellar populations or dust content. The bulge region appears more centrally concentrated, with bluer colors observed in the outer regions of the apparent disk, as well as at the end of the tidal tail. No distinct spiral arm structure is apparent. There may be some evidence of a minor disturbance event occurring.
