The object presents as a galaxy, appearing largely elliptical in morphology, with a generally smooth texture and a high degree of central concentration. The color is predominantly yellow, suggesting an older stellar population with relatively lower rates of on-going star formation. While mostly smooth, there are hints of minor disturbances or faint features, with a trace of a possible disk. These hints imply that the galaxy may have undergone recent or on-going minor interactions. The lack of clearly defined spiral arms or a prominent disk supports its classification as an elliptical galaxy, possibly with a small contribution from star formation activity. The overall roundness of the galactic structure supports the classification as an elliptical rather than a lenticular or spiral galaxy. The galaxy appears relatively isolated, and the presence of disturbances is most likely the effect of internal processes.
