The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. It exhibits a primarily yellowish-white hue, indicative of an older stellar population with a lower rate of recent star formation. The galaxy's shape is generally rounded, appearing somewhat in-between elliptical and circular. There is a possible minor disturbance on the left side of the galaxy, perhaps due to a past or ongoing interaction with a smaller satellite galaxy. Overall, the galaxy seems to be a fairly quiescent system with little evidence of active star formation or major merger events.
