This galaxy presents a morphology suggestive of an ongoing or recent merger event. The primary body displays a relatively smooth texture, with a near-spherical central bulge contributing to the overall roundness. However, a secondary concentration of light is visible, connected to the main structure by a faint bridge or tidal feature. This implies an interaction with a smaller galactic companion. The luminosity is relatively bright and even, suggesting a degree of mixing and active star formation throughout the galactic body. No distinct spiral arms or disk-like features are apparent. The color of the galaxy appears consistent with an older stellar population, and the relative uniform color suggests a lack of dust lanes or significant obscuration. Overall, the structure is complex and disturbed, indicative of dynamical processes associated with the merger. 
