The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated, bright central bulge. The overall color appears to be yellowish-orange, suggesting an older stellar population with fewer young, hot stars. There's little evidence of spiral arms or significant dust lanes. The shape is generally round. There appears to be no major mergers or extreme tidal disturbances influencing the overall morphology, but there may be minor disturbances. The galaxy has a high mass and a very low star formation rate. The galaxy is relatively far away.
