The galaxy appears as a moderately bright, yellowish-white elliptical form. There is evidence of a possible ongoing or recent merger event, with the suggestion of two distinct nuclei or a highly disturbed core region. The galaxy exhibits a generally smooth morphology with little discernible dust or spiral arm structure. Its overall shape is somewhat rounded, although not perfectly spherical. The galaxy exhibits a slight color gradient, appearing marginally bluer towards its outer edges than in the core. No distinct tidal tails are readily visible, suggesting the interaction may be in its later stages or of relatively low mass ratio.
