The galaxy appears to be composed of two distinct luminous components, seemingly gravitationally interacting. The larger, primary component exhibits a smooth morphology, suggestive of an elliptical galaxy. It possesses a somewhat elongated shape, leaning toward a cigar-like structure. The color appears largely yellow-orange, which could indicate a population dominated by older stars. There is a smaller, secondary component located close to the primary galaxy. This appears as a compact and brighter source. Based on the proximity and apparent disturbance to the structure, it is possible that the system may be undergoing a minor merger. Overall, it appears as a fairly massive galaxy, albeit with a relatively low star formation rate. 
