The galaxy appears as a single, relatively smooth object. There is a slight elongation, but overall it is quite round in appearance. No distinct spiral arms or bar structures are readily discernible. The color appears to be primarily yellowish-white, indicating a stellar population that is not dominated by young, blue stars. The lack of significant blue color suggests a low rate of star formation. There is no apparent active galactic nucleus or signs of a recent major merger event. The galaxy displays a concentrated brightness profile. There are some very subtle, minor disturbances in the outer halo region that could indicate a minor merger event in its past.