This galaxy appears to be undergoing an interaction or possible merger. There are two distinct luminous components. The primary component appears relatively smooth and rounded, potentially indicative of an elliptical or lenticular morphology. The other, secondary component is elongated and possibly tidal in nature, suggesting disrupted structure from an interaction. The overall color profile appears yellowish/reddish, suggesting an older stellar population with reduced ongoing star formation. There might be slight disturbances noted in the overall structure. The size is relatively compact.
