The galaxy presents as an elliptical morphology, appearing relatively smooth and concentrated. There is little discernible disk structure. The light profile transitions gradually from the center outwards, with a slightly elongated shape, but trending toward round. The galaxy's core is noticeably brighter and takes on a yellow hue, suggesting an older stellar population that is likely dominant. Evidence of any ongoing major merging activity or significant disturbance is not readily apparent; a minor disturbance cannot be ruled out, as there appears to be some irregular structure in the outer halo. The overall color indicates that star formation may be relatively low compared to the overall galactic mass.
