The galaxy appears to be undergoing a significant merger event. There are two main, luminous components. The larger, primary component exhibits a generally round morphology, indicating a relatively smooth distribution of light, however there is some distortion suggesting tidal effects from the interaction. It presents a yellow-white hue. The secondary component appears more compact, exhibiting a slightly more yellow-orange color. It is located close to the primary galaxy, suggesting strong gravitational interaction. Overall, there are disturbances in the light distribution, indicating ongoing tidal forces and star formation likely triggered by the merger. The system's shape is overall irregular, lacking a well-defined spiral or elliptical structure. The rate of new star creation is relatively low.
