This galaxy exhibits a complex morphology, potentially indicative of an ongoing interaction or recent merger event. Two distinct components are visible. The primary component presents a yellowish hue, suggesting an older stellar population. It appears relatively smooth in texture, possibly an elliptical galaxy or the bulge of a spiral galaxy. The secondary component displays a bluer coloration, implying the presence of younger, hotter stars and active star formation. It appears less defined, possibly a dwarf galaxy.

The overall shape of the system is elongated and asymmetrical, indicating a disruption of the gravitational equilibrium that can be caused by a recent or ongoing merger. There is a faint plume of light that trails in a northern direction. There is likely a presence of dust lanes within this galaxy that are not clearly visible in the optical image. Further observations in different wavelengths, particularly infrared and radio, would be needed to confirm the presence and distribution of dust and gas, and to better understand the dynamics of the system.
