The galaxy presents as a centrally concentrated, elliptical-like system. It exhibits a smooth, largely featureless morphology, with no prominent spiral arms or disk structure readily apparent. The galaxy appears fairly round. The overall color profile is dominated by redder hues, suggestive of an older stellar population and a relatively low rate of on-going star formation. No major merger events are visually indicated. There may be a hint of minor disturbance within the galaxy, but more data is needed to come to any conclusions. 
