The galaxy presents a complex morphology, appearing to be in a state of interaction or merger. Two distinct, bright, yellowish-orange central concentrations are visible, suggesting the presence of two galactic nuclei. These nuclei are embedded within a fainter, more diffuse halo of light. Tidal features, such as faint streams or bridges of stellar material, appear to extend outwards from the central regions, indicating gravitational disturbance and interaction with the galaxy's environment, or the other galactic nuclei. The overall shape of the system is irregular, deviating significantly from a typical spiral or elliptical structure. There is a slight blue tinge to the tidal features. The galaxy's color suggests a relatively old stellar population. Overall, this appears to be a merging system with intermediate mass.
