The object presents as a single galactic structure exhibiting characteristics indicative of an ongoing or recent merger event. The primary body displays a generally elliptical morphology, with a high degree of central concentration. A secondary, smaller concentration of luminosity is observed offset from the primary nucleus, suggesting a second interacting galaxy core. Extended tidal features, or faint disturbed structures, appear to emanate from the main body, further supporting the merger hypothesis. The overall color profile suggests a population of older stars, with a redder appearance. However, there is a small blueish area that is between the two cores. Based on the overall morphology, this system is classified as an interacting galaxy system.
