The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy, exhibiting a concentrated central bulge. It is generally rounded with a slight deviation from perfect circularity, and there is no strong evidence of spiral arm structure. The primary color of the galaxy is yellow, suggestive of an older stellar population with lower levels of ongoing star formation. There may be some minor internal disturbances present but not enough to categorize this galaxy as a merger.
