The galaxy presents as a relatively smooth, elliptical object with a concentrated central bulge. The overall color appears somewhat redder, indicating a population of older stars with lower rates of star formation, suggesting an evolved stellar population. There is a hint of a disk structure but it is poorly defined, and it appears to be a fairly round object. There is a minor indication of disturbance of the shape. There appears to be no evidence of a major merger, but there may be a minor interaction occurring.
