This galaxy presents as a disturbed, merging system. Two primary nuclei are apparent, suggesting an ongoing interaction between two distinct galaxies. Both galactic cores exhibit a yellowish hue, indicative of an older stellar population. Surrounding the central regions, there is a diffuse, less concentrated component with a bluer tint, hinting at more recent star formation activity likely triggered by the ongoing merger event. The overall shape of the system is highly irregular, lacking any clear spiral or elliptical structure. Faint tidal features, possibly stellar streams, are seen extending outwards, further supporting the classification as an interacting or merging system. No distinct bar structure is clearly visible. The bulge appears to be negligible, meaning it is not well defined in comparison to the disk. The overall image suggests a late-stage merger event with significant disruption of the original galactic morphologies.
