The galaxy presents a complex morphology, exhibiting signs of a potential ongoing or recent merger event. Two distinct luminous components are observed, with one being slightly more prominent and centrally located. This brighter component appears relatively smooth and elliptical, with a yellowish-orange hue. The fainter component is located nearby. A faint tidal tail is visible, further suggesting gravitational interaction between the two components. The galaxy exhibits an overall red color, indicative of an older stellar population and potentially lower star formation activity.
