The galaxy appears to be an elliptical galaxy with a smooth morphology, displaying little evidence of spiral arms or distinct features. The light distribution is concentrated toward the center, indicative of a high stellar density in the core region. The galaxy exhibits an elongated shape with some evidence of tidal distortion, possibly indicating a recent or ongoing interaction with a companion galaxy. The color index suggests the presence of an older stellar population with limited ongoing star formation. The galaxy shows signs of a possible ongoing merger event, with some light distortion present. There is evidence of a possible second galactic core very close to the primary, indicating a recent galactic merger event.
