This galaxy exhibits a disturbed morphology, indicative of an ongoing or recent merger event. The central region displays a concentrated luminosity. Extending outward from the center, faint tidal features are discernible, suggesting gravitational interactions. These features are diffuse and appear asymmetric, further supporting the merger scenario. The galaxy presents a complex structure, lacking the defined spiral arms or elliptical shape expected from isolated galaxies. Colors appear to vary with regions of reddish hues visible in the central and likely core regions which may indicate active star formation in a dusty area. Overall, the irregular shape and visible tidal features strongly suggest that this galaxy is currently undergoing a merger with at least one other galaxy.
