The galaxy presents a disturbed morphology, possibly indicative of an ongoing or recent merger event. The light distribution is irregular, with a clumpy appearance across the galaxy. The central region exhibits a relatively high concentration of light. The overall color suggests an older stellar population, although some regions display bluer tinges, potentially pointing to pockets of ongoing star formation. The galaxy is not particularly well-defined, showing evidence of tidal features. There is a likely interaction, or merger, between multiple components.
