The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a concentrated central bulge. The galaxy displays a dominant yellow-orange color, which is likely indicative of an older stellar population with fewer young, massive stars. There is a slight extension in one direction with some possible disruption occurring in the shape and color. There appears to be a small tidal tail, perhaps from a past galactic interaction or merger. Despite this, the galaxy exhibits a fairly relaxed morphology, suggesting that any interaction may have occurred some time ago. Star formation appears to be at a low rate. 
