The galaxy presents with a disturbed morphology, exhibiting signs of a potential ongoing or recent merger event. The central region is somewhat amorphous, lacking a clear, well-defined nucleus. Faint tidal features or extended arms are subtly discernible, hinting at gravitational interactions. The overall color appears relatively uniform, suggesting a mixed stellar population. There is a slight reddish hue in the galaxy indicating some possible dust. The galaxy is largely smooth in appearance, though some irregularities and minor disturbances are present throughout, which is further consistent with interaction.
