The object appears to be a galaxy exhibiting characteristics of a merging or interacting system. Two distinct, yet closely associated, luminous components are visible. The larger, primary component has a smoother, more diffuse appearance, with a yellow-white hue suggestive of an older stellar population, possibly with an elliptical morphology. The second, smaller component shows a bluer tint, which may indicate more recent star formation activity. There seems to be a bridge of material connecting the two components, potentially a tidal tail resulting from gravitational interaction. Overall, the system shows signs of disturbance, with the primary component appearing less structured than a typical elliptical galaxy. The system's colour profile indicates a range of stellar ages within each component.
