The galaxy presents an overall reddish-yellow hue, indicative of a stellar population dominated by older, redder stars. It exhibits a central bulge region that appears relatively smooth and centrally concentrated, with an overall elliptical shape. A faint, disk-like structure is visible extending from the bulge. There is a hint of asymmetric structure that could indicate a minor interaction or disturbance. The absence of strong blue regions suggests relatively low ongoing star formation. Overall the galaxy seems to be fairly massive. 
