The galaxy presents as a somewhat irregular, diffuse structure with a generally elongated morphology. There is evidence of a central concentration of light, suggesting a nucleus, though it is not particularly distinct. The overall color appears bluish, especially around the central area, which indicates the presence of younger stellar populations and ongoing star formation.

The galaxy exhibits signs of possible interaction or disturbance. The morphology is asymmetric, with extended features that could be tidal tails or disrupted arms. There also may be evidence of a minor companion galaxy or a tidal dwarf galaxy forming. These disturbances suggest recent or ongoing interactions with another galaxy. The galaxy may be undergoing a merging event.
