The galaxy presents an overall elliptical appearance, with a moderate degree of smoothness. A defined central bulge is visible, appearing brighter and more condensed than the surrounding galactic disk. There is evidence of a disk-like structure extending outwards from the bulge. The disk exhibits subtle features or disturbances, possibly suggesting minor interactions or internal activity. A faint tidal stream or a possible minor merger appears to be present near the central bulge. The galaxy does not show strong indications of a major merger event. 
