The galaxy exhibits a morphology indicative of an ongoing or recent merger event. Two distinct luminous cores are visible, with one displaying a brighter, more concentrated intensity profile and a slightly bluer color compared to the other. The second core presents a more diffuse appearance and a comparatively redder hue, suggestive of an older stellar population. The surrounding galactic material exhibits a complex, disturbed structure, appearing less defined and with irregular extensions, suggesting tidal interactions are at play. The overall shape deviates substantially from a regular elliptical or spiral form, indicating a dynamic system influenced by gravitational interactions. There is no discernible disk-like structure or spiral arm morphology present.
