This galaxy appears to be undergoing a significant interaction, possibly a merger. It presents a somewhat irregular morphology. The primary body of the galaxy exhibits a relatively smooth light distribution, with a centrally concentrated core. There is some indication of tidal features extending outwards, suggesting gravitational disturbance due to the interaction. The galaxy displays a color gradient, appearing bluer in the outer regions and redder towards the core. This suggests a potential difference in stellar populations, with younger, bluer stars possibly dominating the outer regions where star formation may be more active. There is a distinct secondary object in proximity to the primary galaxy, with a more compact, round shape. It is possible this is a smaller galaxy in the process of merging. Some disturbance in the surrounding area may be present.
