The galaxy presents as a relatively small, elliptical object. The core exhibits a high degree of red-shifted light, indicating a potential concentration of older stellar populations or significant dust obscuration. Surrounding the core is a distinct ring-like structure featuring a complex interplay of colors. There appear to be blue and green emissions within the ring, suggesting the presence of younger, hotter stars, possibly indicative of recent star formation. Furthermore, the presence of disturbances suggests the possibility of minor interaction with another galaxy. The galaxy does not appear to be undergoing a major merging event; however, some internal asymmetries may suggest minor tidal interactions or internal dynamic processes. Overall, the galaxy presents a system with both old and potentially newer stellar components, with a possible merger occurring.
