The galaxy presents as a complex system, with evidence of possible interaction or merging. It appears as an elliptical formation with a central bulge that shows a concentrated luminosity gradient. The light profile suggests that the galaxy could have an obscured disc component with a non-uniform distribution of stellar populations or dust lanes contributing to the colour variations observed. The outer regions show a lower surface brightness, fading into the background. A secondary bright object located within the primary object's diffuse halo could represent an ongoing merger event or a distinct foreground object not associated with the main galaxy. The overall colour distribution of the main galaxy appears relatively homogeneous with slight shifts towards redder tones in the central region and blue shifts outside this area. Based on observed features, it is possible that this is a merging binary system, but additional data would be needed to be certain.
