The galaxy appears to be an elliptical or lenticular galaxy, exhibiting a generally smooth and rounded morphology. It is not a clear spiral structure. The color indices suggest a population dominated by older stars, indicating relatively little ongoing star formation. The galaxy seems to be undergoing some form of merging or tidal interaction. The light distribution is centrally concentrated. There may be a companion galaxy that is in the process of merging. The isophotes appear generally regular.
