The galaxy exhibits a disturbed morphology, possibly indicative of an ongoing or recent merger event. There are two distinct color populations present. One is a bluer, elongated region, and the other is a yellower, more compact region. The bluer region displays an irregular structure, suggesting active star formation or tidal disruption due to gravitational interaction. The yellower region appears to be a more evolved stellar population. It has a smoother profile, potentially representing the remnant core of one of the merging galaxies. There also seems to be faint, diffuse light extending from the blue region, possibly indicating a tidal tail or bridge formed during the interaction. Overall, the system suggests a complex history of gravitational interaction.
