The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that gradually diffuses outwards. There appears to be a blueish hue in the outer parts of the galaxy, suggesting the presence of some recent star formation in a disk structure. The galaxy is not perfectly rounded, showing a slight elongation. There is no indication of any major ongoing mergers. There may be some minor disturbances apparent in the structure, although it is difficult to distinguish.
