The galaxy presents a complex morphology, exhibiting features suggestive of an ongoing or recent merger event. A central, bright, and somewhat concentrated bulge dominates the core region, appearing yellowish-orange in color, which likely indicates an older stellar population. Emanating from this central region, there's evidence of a disrupted or distorted disk-like structure. One section of the disk appears somewhat smooth, while another exhibits filamentary extensions or tidal tails, indicating gravitational interactions. There is some asymmetry in the overall shape; one side is more extended, while the other is more compact. There is also a bluer tinge to the galaxy, potentially indicating star forming regions.
