The galaxy exhibits a morphology that appears largely smooth, with a concentrated central bulge, suggesting an elliptical or lenticular galaxy type. The color is predominantly yellow-orange, indicative of an older stellar population with diminished recent star formation. A slight elongation is observed, with evidence of potential tidal disruption. The galaxy displays no prominent spiral arm structure, but there are subtle irregularities or disturbances that could be indicative of a past or ongoing interaction. The overall appearance indicates a galaxy that is relatively massive. The image shows a galaxy that may be currently undergoing a merger, with a large portion appearing to have been disrupted, with an overall red hue.
