The galaxy presents an elliptical morphology, appearing largely smooth in structure with a dominant central bulge. There is a very slight disk component. The color of the central bulge is yellowish, suggesting an older stellar population. There are faint, slightly bluer outer regions, potentially indicating more recent, albeit low-level, star formation activity. The overall shape is not perfectly round, leaning towards a slight ellipticity. There is no immediately visible evidence of major merging events, although there is a slight irregular outer structure. The apparent angular size of the galaxy is quite small, which indicates the galaxy is at a considerable distance.
