The galaxy appears to be a relatively smooth, elliptical-like structure with a concentrated central bulge. The overall shape is generally round. There is no discernible spiral arm structure. A slight colour gradient is present, transitioning from a more yellowish-white core to a subtly redder outer halo. No significant dust lanes or active star-forming regions are immediately apparent. The galaxy appears relatively isolated, showing only faint signs of minor disturbances, as though there is little interaction with neighboring objects. It's estimated to be of an intermediate mass range and low specific star formation rate.
