The galaxy presents as a luminous object with a complex morphology suggestive of an ongoing or recent merger event. The central region exhibits a concentrated luminosity, appearing nearly spherical and unresolved at this resolution. Emanating from this central region is a prominent tidal tail that extends in a curved trajectory. The tail displays a bluer hue compared to the central region, possibly indicating the presence of younger stars and ongoing star formation within. The overall shape of the galaxy departs significantly from a regular elliptical or spiral structure, exhibiting signs of significant gravitational disturbance. The elongated shape of the tidal tail and the amorphous structure of the main body contribute to this assessment. Evidence of multiple merging events is hard to deny as the center of the galaxy is distorted.
