The galaxy presents a morphology that suggests a system undergoing a significant interaction or merger. There appears to be two distinct, bright central concentrations of light, indicative of either two galactic nuclei in close proximity or a single nucleus with a strong bar feature. A faint, diffuse halo of light surrounds the central region, displaying a non-uniform distribution. This suggests tidal disturbances possibly caused by gravitational interactions. The overall shape of the galaxy deviates substantially from a smooth, elliptical form. Irregularities are observed in the outer regions, which may indicate ongoing tidal stripping of stellar material. Patches of slightly bluer light can be discerned, potentially suggesting regions of star formation activity triggered by the interaction/merger event. There may be minor disturbances surrounding the galaxy itself.
