The object presents as a relatively smooth, concentrated mass of light, appearing mostly round with a slight suggestion of elongation. The light is predominantly yellow-orange, indicative of an older stellar population. There is some evidence of a possible interaction or merger event. It shows two distinct, rounded bright spots, close together. The object appears to be a quiescent galaxy with little ongoing star formation. This is further supported by the smooth morphology and lack of discernible spiral arms or active star-forming regions. There appears to be an absence of any disk-like structure. The overall morphology is consistent with an elliptical galaxy or perhaps a spiral galaxy undergoing a significant merger event, leaving a remnant compact object.
