The galaxy appears as a somewhat disturbed system with a complex morphology, potentially a merger in progress. It displays a prominent central bulge that is slightly elongated and features a bright, concentrated core. There are hints of disturbed tidal features and faint, diffuse outer regions, which point towards gravitational interactions. These features indicate a system with a high likelihood of past or ongoing mergers. The color distribution suggests a population of older stars with little active star formation throughout the majority of the galaxy. The overall morphology does not clearly present any defined spiral or elliptical characteristics. The system measures approximately 6 kiloparsecs across. The galaxy appears to be experiencing some disruption to its shape, indicating an unstable configuration.
