The galaxy presents a generally smooth morphology. The light distribution suggests a concentrated central region, possibly a bulge, surrounded by a more diffuse halo. The shape appears largely rounded, deviating slightly from perfect circularity. There is evidence suggesting an ongoing interaction or merger with another galactic object, marked by a notable tidal disturbance. The galaxy exhibits a color gradient, transitioning from bluer hues in the outer regions to redder tones towards the center, which might imply differential stellar populations or dust distribution. The object’s overall luminosity indicates a galaxy of substantial size and mass. Star formation appears to be active.
