The galaxy appears to be a relatively smooth elliptical type. It exhibits a concentrated central bulge that is nearly spherical and very bright, with a significant decrease in luminosity towards the outer regions. There is a slight elongation to the shape of the galaxy, suggesting it's not perfectly spherical. The overall light profile indicates that the galaxy is relatively undisturbed, with no obvious signs of major mergers or tidal interactions. No distinct spiral arm features are observed; the galaxy appears to be composed of older stellar populations, indicated by its color. There are no apparent dust lanes or regions of active star formation visible within the galaxy. There is some indication of minor disturbances to the disk, but not significant.
