The galaxy presents a generally smooth and elliptical morphology. The central region exhibits a concentrated, bright, yellowish core, possibly indicative of an older stellar population and/or a supermassive black hole. The galaxy appears to be relatively undisturbed, showing no signs of major mergers or significant tidal disruptions. The outer regions display a subtle decrease in luminosity. The galaxy is slightly elongated, with a suggestion of a disk-like structure, though the smoothness of the light distribution suggests it is not a well-defined spiral galaxy. There is a subtle blue hue in the outer regions which suggests the possibility of some ongoing star formation, though minimal, in this galaxy.
