The galaxy presents a complex morphology suggesting an ongoing or recent interaction. A bright, relatively compact core is observed, exhibiting a concentrated region of high luminosity. Emanating from this central core is an extended, less defined structure. This structure appears diffuse and irregular, potentially indicating tidal debris or disrupted galactic material. The color gradient within the extended structure suggests varying stellar populations or dust distribution, with bluer regions possibly indicating areas of active star formation and redder regions potentially indicating older stellar populations or dust obscuration. There is evidence of possible merger activity with a faint tail like shape, and the general shape of the galaxy is irregular. The overall appearance suggests a system undergoing gravitational disturbance, possibly due to a merger or tidal interaction with another galaxy.
