The galaxy exhibits a disturbed morphology, indicative of an ongoing or recent interaction. The core region appears to be composed of two distinct, bright nuclei embedded within a diffuse, yellowish halo. This suggests either a close binary system or an advanced stage of galactic merger. Faint tidal tails or streams of stellar material extend outwards, further supporting the interaction scenario. The overall color suggests a mix of stellar populations, with older, yellow stars dominating the central bulge and hints of bluer stars in the tails, potentially indicating regions of active star formation triggered by the interaction. Dust lanes or obscurations may be present, contributing to the patchy appearance. 
